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.
Autor*in: |
Williams, P. S. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
1975 |
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Schlagwörter: |
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Anmerkung: |
© D. Reidel Publishing Company 1975 |
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Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 34(1975), 2 vom: Mai, Seite 425-430 |
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Übergeordnetes Werk: |
volume:34 ; year:1975 ; number:2 ; month:05 ; pages:425-430 |
Links: |
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DOI / URN: |
10.1007/BF00644810 |
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Katalog-ID: |
OLC2066124117 |
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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 |
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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 |
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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 |
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