Problems with the interpretation of the 220 nm interstellar feature

Abstract The bump in the ultraviolet part of the interstellar extinction curve provides a great challenge in the modelling of interstellar dust. Its shape can be well approximated by a classical dispersion profile with a total halfwidth of 48 nm centred at 217 nm. Apart from few slightly deviating c...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Friedemann, C. [verfasserIn] Gürtler, J.

Format:	Artikel
Sprache:	Englisch

Erschienen:	1986

Schlagwörter:	Colour Dust Graphite Final Decision Conclusive Result

Anmerkung:	© D. Reidel Publishing Company 1986

Übergeordnetes Werk:	Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 128(1986), 1 vom: Dez., Seite 71-81
Übergeordnetes Werk:	volume:128 ; year:1986 ; number:1 ; month:12 ; pages:71-81

Links:	Volltext

DOI / URN:	10.1007/BF00656019

Katalog-ID:	OLC2066163686

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allfields	10.1007/BF00656019 doi (DE-627)OLC2066163686 (DE-He213)BF00656019-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Friedemann, C. verfasserin aut Problems with the interpretation of the 220 nm interstellar feature 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract The bump in the ultraviolet part of the interstellar extinction curve provides a great challenge in the modelling of interstellar dust. Its shape can be well approximated by a classical dispersion profile with a total halfwidth of 48 nm centred at 217 nm. Apart from few slightly deviating cases the parameters of the band seem to be surprisingly constant in the solar neighbourhood. The equivalent widthW of the 217 nm band shows a very tight correlation with the colour excessE(B-V). Studies of correlations with the strength of diffuse interstellar bands gave no conclusive results as to the nature of the band. The most common interpretation of the 217 nm feature as originating from small graphite grians meets several difficulties. No final decision on the carrier can be made at present. Colour Dust Graphite Final Decision Conclusive Result Gürtler, J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 128(1986), 1 vom: Dez., Seite 71-81 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:128 year:1986 number:1 month:12 pages:71-81 https://doi.org/10.1007/BF00656019 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_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 128 1986 1 12 71-81
spelling	10.1007/BF00656019 doi (DE-627)OLC2066163686 (DE-He213)BF00656019-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Friedemann, C. verfasserin aut Problems with the interpretation of the 220 nm interstellar feature 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract The bump in the ultraviolet part of the interstellar extinction curve provides a great challenge in the modelling of interstellar dust. Its shape can be well approximated by a classical dispersion profile with a total halfwidth of 48 nm centred at 217 nm. Apart from few slightly deviating cases the parameters of the band seem to be surprisingly constant in the solar neighbourhood. The equivalent widthW of the 217 nm band shows a very tight correlation with the colour excessE(B-V). Studies of correlations with the strength of diffuse interstellar bands gave no conclusive results as to the nature of the band. The most common interpretation of the 217 nm feature as originating from small graphite grians meets several difficulties. No final decision on the carrier can be made at present. Colour Dust Graphite Final Decision Conclusive Result Gürtler, J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 128(1986), 1 vom: Dez., Seite 71-81 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:128 year:1986 number:1 month:12 pages:71-81 https://doi.org/10.1007/BF00656019 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_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 128 1986 1 12 71-81
allfields_unstemmed	10.1007/BF00656019 doi (DE-627)OLC2066163686 (DE-He213)BF00656019-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Friedemann, C. verfasserin aut Problems with the interpretation of the 220 nm interstellar feature 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract The bump in the ultraviolet part of the interstellar extinction curve provides a great challenge in the modelling of interstellar dust. Its shape can be well approximated by a classical dispersion profile with a total halfwidth of 48 nm centred at 217 nm. Apart from few slightly deviating cases the parameters of the band seem to be surprisingly constant in the solar neighbourhood. The equivalent widthW of the 217 nm band shows a very tight correlation with the colour excessE(B-V). Studies of correlations with the strength of diffuse interstellar bands gave no conclusive results as to the nature of the band. The most common interpretation of the 217 nm feature as originating from small graphite grians meets several difficulties. No final decision on the carrier can be made at present. Colour Dust Graphite Final Decision Conclusive Result Gürtler, J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 128(1986), 1 vom: Dez., Seite 71-81 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:128 year:1986 number:1 month:12 pages:71-81 https://doi.org/10.1007/BF00656019 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_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 128 1986 1 12 71-81
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allfieldsSound	10.1007/BF00656019 doi (DE-627)OLC2066163686 (DE-He213)BF00656019-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Friedemann, C. verfasserin aut Problems with the interpretation of the 220 nm interstellar feature 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract The bump in the ultraviolet part of the interstellar extinction curve provides a great challenge in the modelling of interstellar dust. Its shape can be well approximated by a classical dispersion profile with a total halfwidth of 48 nm centred at 217 nm. Apart from few slightly deviating cases the parameters of the band seem to be surprisingly constant in the solar neighbourhood. The equivalent widthW of the 217 nm band shows a very tight correlation with the colour excessE(B-V). Studies of correlations with the strength of diffuse interstellar bands gave no conclusive results as to the nature of the band. The most common interpretation of the 217 nm feature as originating from small graphite grians meets several difficulties. No final decision on the carrier can be made at present. Colour Dust Graphite Final Decision Conclusive Result Gürtler, J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 128(1986), 1 vom: Dez., Seite 71-81 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:128 year:1986 number:1 month:12 pages:71-81 https://doi.org/10.1007/BF00656019 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_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 128 1986 1 12 71-81
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title_auth	Problems with the interpretation of the 220 nm interstellar feature
abstract	Abstract The bump in the ultraviolet part of the interstellar extinction curve provides a great challenge in the modelling of interstellar dust. Its shape can be well approximated by a classical dispersion profile with a total halfwidth of 48 nm centred at 217 nm. Apart from few slightly deviating cases the parameters of the band seem to be surprisingly constant in the solar neighbourhood. The equivalent widthW of the 217 nm band shows a very tight correlation with the colour excessE(B-V). Studies of correlations with the strength of diffuse interstellar bands gave no conclusive results as to the nature of the band. The most common interpretation of the 217 nm feature as originating from small graphite grians meets several difficulties. No final decision on the carrier can be made at present. © D. Reidel Publishing Company 1986
abstractGer	Abstract The bump in the ultraviolet part of the interstellar extinction curve provides a great challenge in the modelling of interstellar dust. Its shape can be well approximated by a classical dispersion profile with a total halfwidth of 48 nm centred at 217 nm. Apart from few slightly deviating cases the parameters of the band seem to be surprisingly constant in the solar neighbourhood. The equivalent widthW of the 217 nm band shows a very tight correlation with the colour excessE(B-V). Studies of correlations with the strength of diffuse interstellar bands gave no conclusive results as to the nature of the band. The most common interpretation of the 217 nm feature as originating from small graphite grians meets several difficulties. No final decision on the carrier can be made at present. © D. Reidel Publishing Company 1986
abstract_unstemmed	Abstract The bump in the ultraviolet part of the interstellar extinction curve provides a great challenge in the modelling of interstellar dust. Its shape can be well approximated by a classical dispersion profile with a total halfwidth of 48 nm centred at 217 nm. Apart from few slightly deviating cases the parameters of the band seem to be surprisingly constant in the solar neighbourhood. The equivalent widthW of the 217 nm band shows a very tight correlation with the colour excessE(B-V). Studies of correlations with the strength of diffuse interstellar bands gave no conclusive results as to the nature of the band. The most common interpretation of the 217 nm feature as originating from small graphite grians meets several difficulties. No final decision on the carrier can be made at present. © D. Reidel Publishing Company 1986
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container_issue	1
title_short	Problems with the interpretation of the 220 nm interstellar feature
url	https://doi.org/10.1007/BF00656019
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author2	Gürtler, J.
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doi_str	10.1007/BF00656019
up_date	2024-07-04T03:53:55.633Z
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