A note on critically rotating polytropes

Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations.

Gespeichert in:

Autor*in:	Williams, P. S. [verfasserIn]

Format:	Artikel
Sprache:	Englisch

Erschienen:	1975

Schlagwörter:	Approximation Scheme Structure Calculation Stellar Model Stellar Structure

Anmerkung:	© D. Reidel Publishing Company 1975

Übergeordnetes Werk:	Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 34(1975), 2 vom: Mai, Seite 425-430
Übergeordnetes Werk:	volume:34 ; year:1975 ; number:2 ; month:05 ; pages:425-430

Links:	Volltext

DOI / URN:	10.1007/BF00644810

Katalog-ID:	OLC2066124117

Internformat


LEADER	01000caa a22002652 4500
001	OLC2066124117
003	DE-627
005	20230502211415.0
007	tu
008	200820s1975 xx \|\|\|\|\| 00\| \|\|eng c
024	7		\|a 10.1007/BF00644810 \|2 doi
035			\|a (DE-627)OLC2066124117
035			\|a (DE-He213)BF00644810-p
040			\|a DE-627 \|b ger \|c DE-627 \|e rakwb
041			\|a eng
082	0	4	\|a 520 \|a 530 \|a 620 \|q VZ
084			\|a 16,12 \|2 ssgn
100	1		\|a Williams, P. S. \|e verfasserin \|4 aut
245	1	0	\|a A note on critically rotating polytropes
264		1	\|c 1975
336			\|a Text \|b txt \|2 rdacontent
337			\|a ohne Hilfsmittel zu benutzen \|b n \|2 rdamedia
338			\|a Band \|b nc \|2 rdacarrier
500			\|a © D. Reidel Publishing Company 1975
520			\|a Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations.
650		4	\|a Approximation Scheme
650		4	\|a Structure Calculation
650		4	\|a Stellar Model
650		4	\|a Stellar Structure
773	0	8	\|i Enthalten in \|t Astrophysics and space science \|d Kluwer Academic Publishers, 1968 \|g 34(1975), 2 vom: Mai, Seite 425-430 \|w (DE-627)129062723 \|w (DE-600)629-4 \|w (DE-576)014393522 \|x 0004-640X \|7 nnns
773	1	8	\|g volume:34 \|g year:1975 \|g number:2 \|g month:05 \|g pages:425-430
856	4	1	\|u https://doi.org/10.1007/BF00644810 \|z lizenzpflichtig \|3 Volltext
912			\|a GBV_USEFLAG_A
912			\|a SYSFLAG_A
912			\|a GBV_OLC
912			\|a SSG-OLC-TEC
912			\|a SSG-OLC-PHY
912			\|a SSG-OLC-AST
912			\|a SSG-OPC-AST
912			\|a GBV_ILN_11
912			\|a GBV_ILN_20
912			\|a GBV_ILN_21
912			\|a GBV_ILN_22
912			\|a GBV_ILN_24
912			\|a GBV_ILN_31
912			\|a GBV_ILN_40
912			\|a GBV_ILN_47
912			\|a GBV_ILN_70
912			\|a GBV_ILN_601
912			\|a GBV_ILN_2002
912			\|a GBV_ILN_2279
912			\|a GBV_ILN_2286
912			\|a GBV_ILN_4012
912			\|a GBV_ILN_4035
912			\|a GBV_ILN_4046
912			\|a GBV_ILN_4082
912			\|a GBV_ILN_4103
912			\|a GBV_ILN_4306
912			\|a GBV_ILN_4700
951			\|a AR
952			\|d 34 \|j 1975 \|e 2 \|c 05 \|h 425-430

Indexfelder

author_variant	p s w ps psw
matchkey_str	article:0004640X:1975----::ntociialrttn
hierarchy_sort_str	1975
publishDate	1975
allfields	10.1007/BF00644810 doi (DE-627)OLC2066124117 (DE-He213)BF00644810-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Williams, P. S. verfasserin aut A note on critically rotating polytropes 1975 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1975 Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations. Approximation Scheme Structure Calculation Stellar Model Stellar Structure Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 34(1975), 2 vom: Mai, Seite 425-430 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:34 year:1975 number:2 month:05 pages:425-430 https://doi.org/10.1007/BF00644810 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 34 1975 2 05 425-430
spelling	10.1007/BF00644810 doi (DE-627)OLC2066124117 (DE-He213)BF00644810-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Williams, P. S. verfasserin aut A note on critically rotating polytropes 1975 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1975 Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations. Approximation Scheme Structure Calculation Stellar Model Stellar Structure Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 34(1975), 2 vom: Mai, Seite 425-430 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:34 year:1975 number:2 month:05 pages:425-430 https://doi.org/10.1007/BF00644810 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 34 1975 2 05 425-430
allfields_unstemmed	10.1007/BF00644810 doi (DE-627)OLC2066124117 (DE-He213)BF00644810-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Williams, P. S. verfasserin aut A note on critically rotating polytropes 1975 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1975 Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations. Approximation Scheme Structure Calculation Stellar Model Stellar Structure Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 34(1975), 2 vom: Mai, Seite 425-430 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:34 year:1975 number:2 month:05 pages:425-430 https://doi.org/10.1007/BF00644810 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 34 1975 2 05 425-430
allfieldsGer	10.1007/BF00644810 doi (DE-627)OLC2066124117 (DE-He213)BF00644810-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Williams, P. S. verfasserin aut A note on critically rotating polytropes 1975 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1975 Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations. Approximation Scheme Structure Calculation Stellar Model Stellar Structure Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 34(1975), 2 vom: Mai, Seite 425-430 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:34 year:1975 number:2 month:05 pages:425-430 https://doi.org/10.1007/BF00644810 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 34 1975 2 05 425-430
allfieldsSound	10.1007/BF00644810 doi (DE-627)OLC2066124117 (DE-He213)BF00644810-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Williams, P. S. verfasserin aut A note on critically rotating polytropes 1975 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1975 Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations. Approximation Scheme Structure Calculation Stellar Model Stellar Structure Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 34(1975), 2 vom: Mai, Seite 425-430 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:34 year:1975 number:2 month:05 pages:425-430 https://doi.org/10.1007/BF00644810 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 34 1975 2 05 425-430
language	English
source	Enthalten in Astrophysics and space science 34(1975), 2 vom: Mai, Seite 425-430 volume:34 year:1975 number:2 month:05 pages:425-430
sourceStr	Enthalten in Astrophysics and space science 34(1975), 2 vom: Mai, Seite 425-430 volume:34 year:1975 number:2 month:05 pages:425-430
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Approximation Scheme Structure Calculation Stellar Model Stellar Structure
dewey-raw	520
isfreeaccess_bool	false
container_title	Astrophysics and space science
authorswithroles_txt_mv	Williams, P. S. @@aut@@
publishDateDaySort_date	1975-05-01T00:00:00Z
hierarchy_top_id	129062723
dewey-sort	3520
id	OLC2066124117
language_de	englisch
fullrecord	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2066124117</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502211415.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s1975 xx \|\|\|\|\| 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF00644810</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066124117</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF00644810-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Williams, P. S.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">A note on critically rotating polytropes</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1975</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© D. Reidel Publishing Company 1975</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Approximation Scheme</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Structure Calculation</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stellar Model</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stellar Structure</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Astrophysics and space science</subfield><subfield code="d">Kluwer Academic Publishers, 1968</subfield><subfield code="g">34(1975), 2 vom: Mai, Seite 425-430</subfield><subfield code="w">(DE-627)129062723</subfield><subfield code="w">(DE-600)629-4</subfield><subfield code="w">(DE-576)014393522</subfield><subfield code="x">0004-640X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:34</subfield><subfield code="g">year:1975</subfield><subfield code="g">number:2</subfield><subfield code="g">month:05</subfield><subfield code="g">pages:425-430</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF00644810</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_21</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_601</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4035</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4082</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4103</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">34</subfield><subfield code="j">1975</subfield><subfield code="e">2</subfield><subfield code="c">05</subfield><subfield code="h">425-430</subfield></datafield></record></collection>
author	Williams, P. S.
spellingShingle	Williams, P. S. ddc 520 ssgn 16,12 misc Approximation Scheme misc Structure Calculation misc Stellar Model misc Stellar Structure A note on critically rotating polytropes
authorStr	Williams, P. S.
ppnlink_with_tag_str_mv	@@773@@(DE-627)129062723
format	Article
dewey-ones	520 - Astronomy & allied sciences 530 - Physics 620 - Engineering & allied operations
delete_txt_mv	keep
author_role	aut
collection	OLC
remote_str	false
illustrated	Not Illustrated
issn	0004-640X
topic_title	520 530 620 VZ 16,12 ssgn A note on critically rotating polytropes Approximation Scheme Structure Calculation Stellar Model Stellar Structure
topic	ddc 520 ssgn 16,12 misc Approximation Scheme misc Structure Calculation misc Stellar Model misc Stellar Structure
topic_unstemmed	ddc 520 ssgn 16,12 misc Approximation Scheme misc Structure Calculation misc Stellar Model misc Stellar Structure
topic_browse	ddc 520 ssgn 16,12 misc Approximation Scheme misc Structure Calculation misc Stellar Model misc Stellar Structure
format_facet	Aufsätze Gedruckte Aufsätze
format_main_str_mv	Text Zeitschrift/Artikel
carriertype_str_mv	nc
hierarchy_parent_title	Astrophysics and space science
hierarchy_parent_id	129062723
dewey-tens	520 - Astronomy 530 - Physics 620 - Engineering
hierarchy_top_title	Astrophysics and space science
isfreeaccess_txt	false
familylinks_str_mv	(DE-627)129062723 (DE-600)629-4 (DE-576)014393522
title	A note on critically rotating polytropes
ctrlnum	(DE-627)OLC2066124117 (DE-He213)BF00644810-p
title_full	A note on critically rotating polytropes
author_sort	Williams, P. S.
journal	Astrophysics and space science
journalStr	Astrophysics and space science
lang_code	eng
isOA_bool	false
dewey-hundreds	500 - Science 600 - Technology
recordtype	marc
publishDateSort	1975
contenttype_str_mv	txt
container_start_page	425
author_browse	Williams, P. S.
container_volume	34
class	520 530 620 VZ 16,12 ssgn
format_se	Aufsätze
author-letter	Williams, P. S.
doi_str_mv	10.1007/BF00644810
dewey-full	520 530 620
title_sort	a note on critically rotating polytropes
title_auth	A note on critically rotating polytropes
abstract	Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations. © D. Reidel Publishing Company 1975
abstractGer	Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations. © D. Reidel Publishing Company 1975
abstract_unstemmed	Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations. © D. Reidel Publishing Company 1975
collection_details	GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700
container_issue	2
title_short	A note on critically rotating polytropes
url	https://doi.org/10.1007/BF00644810
remote_bool	false
ppnlink	129062723
mediatype_str_mv	n
isOA_txt	false
hochschulschrift_bool	false
doi_str	10.1007/BF00644810
up_date	2024-07-04T03:49:08.215Z
_version_	1803618823140540416
fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2066124117</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502211415.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s1975 xx \|\|\|\|\| 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF00644810</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066124117</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF00644810-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Williams, P. S.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">A note on critically rotating polytropes</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1975</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© D. Reidel Publishing Company 1975</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The structure of critically rotating polytropes is calculated using two (reated) Roche-type approximation schemes, one of which has been developed for stellar models. Comparisons with other results are made as a validation of these methods in stellar structure calculations.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Approximation Scheme</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Structure Calculation</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stellar Model</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stellar Structure</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Astrophysics and space science</subfield><subfield code="d">Kluwer Academic Publishers, 1968</subfield><subfield code="g">34(1975), 2 vom: Mai, Seite 425-430</subfield><subfield code="w">(DE-627)129062723</subfield><subfield code="w">(DE-600)629-4</subfield><subfield code="w">(DE-576)014393522</subfield><subfield code="x">0004-640X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:34</subfield><subfield code="g">year:1975</subfield><subfield code="g">number:2</subfield><subfield code="g">month:05</subfield><subfield code="g">pages:425-430</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF00644810</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_21</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_601</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4035</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4082</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4103</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">34</subfield><subfield code="j">1975</subfield><subfield code="e">2</subfield><subfield code="c">05</subfield><subfield code="h">425-430</subfield></datafield></record></collection>
score	7.3998165

Nicht das Richtige dabei?

Schreiben Sie uns!

A note on critically rotating polytropes

Nicht das Richtige dabei?

Zugang & Verfügbarkeit

Vorhandene Bände

Nicht das Richtige dabei?