Multi-frequency observations of the 1985 outburst of RS ophiuchi
Abstract The 1985 outburst of the bright, recurrent nova RS Oph was almost simultaneously observed at X-ray, UV, optical, IR and radio frequencies at many epochs. The abundances in the ejected shell and the development of the bolometric luminosity as a function of time suggest that the cause of the...
Ausführliche Beschreibung
Autor*in: |
Snijders, M. A. J. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
1987 |
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Schlagwörter: |
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Anmerkung: |
© D. Reidel Publishing Company 1987 |
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Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 130(1987), 1-2 vom: Feb., Seite 243-254 |
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Übergeordnetes Werk: |
volume:130 ; year:1987 ; number:1-2 ; month:02 ; pages:243-254 |
Links: |
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DOI / URN: |
10.1007/BF00655002 |
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Katalog-ID: |
OLC2066164593 |
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10.1007/BF00655002 doi (DE-627)OLC2066164593 (DE-He213)BF00655002-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Snijders, M. A. J. verfasserin aut Multi-frequency observations of the 1985 outburst of RS ophiuchi 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract The 1985 outburst of the bright, recurrent nova RS Oph was almost simultaneously observed at X-ray, UV, optical, IR and radio frequencies at many epochs. The abundances in the ejected shell and the development of the bolometric luminosity as a function of time suggest that the cause of the outburst is a nuclear runaway on a massive white dwarf. Radio Frequency White Dwarf Bolometric Luminosity Massive White Dwarf Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 130(1987), 1-2 vom: Feb., Seite 243-254 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:130 year:1987 number:1-2 month:02 pages:243-254 https://doi.org/10.1007/BF00655002 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 130 1987 1-2 02 243-254 |
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10.1007/BF00655002 doi (DE-627)OLC2066164593 (DE-He213)BF00655002-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Snijders, M. A. J. verfasserin aut Multi-frequency observations of the 1985 outburst of RS ophiuchi 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract The 1985 outburst of the bright, recurrent nova RS Oph was almost simultaneously observed at X-ray, UV, optical, IR and radio frequencies at many epochs. The abundances in the ejected shell and the development of the bolometric luminosity as a function of time suggest that the cause of the outburst is a nuclear runaway on a massive white dwarf. Radio Frequency White Dwarf Bolometric Luminosity Massive White Dwarf Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 130(1987), 1-2 vom: Feb., Seite 243-254 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:130 year:1987 number:1-2 month:02 pages:243-254 https://doi.org/10.1007/BF00655002 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 130 1987 1-2 02 243-254 |
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10.1007/BF00655002 doi (DE-627)OLC2066164593 (DE-He213)BF00655002-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Snijders, M. A. J. verfasserin aut Multi-frequency observations of the 1985 outburst of RS ophiuchi 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract The 1985 outburst of the bright, recurrent nova RS Oph was almost simultaneously observed at X-ray, UV, optical, IR and radio frequencies at many epochs. The abundances in the ejected shell and the development of the bolometric luminosity as a function of time suggest that the cause of the outburst is a nuclear runaway on a massive white dwarf. Radio Frequency White Dwarf Bolometric Luminosity Massive White Dwarf Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 130(1987), 1-2 vom: Feb., Seite 243-254 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:130 year:1987 number:1-2 month:02 pages:243-254 https://doi.org/10.1007/BF00655002 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 130 1987 1-2 02 243-254 |
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10.1007/BF00655002 doi (DE-627)OLC2066164593 (DE-He213)BF00655002-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Snijders, M. A. J. verfasserin aut Multi-frequency observations of the 1985 outburst of RS ophiuchi 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract The 1985 outburst of the bright, recurrent nova RS Oph was almost simultaneously observed at X-ray, UV, optical, IR and radio frequencies at many epochs. The abundances in the ejected shell and the development of the bolometric luminosity as a function of time suggest that the cause of the outburst is a nuclear runaway on a massive white dwarf. Radio Frequency White Dwarf Bolometric Luminosity Massive White Dwarf Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 130(1987), 1-2 vom: Feb., Seite 243-254 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:130 year:1987 number:1-2 month:02 pages:243-254 https://doi.org/10.1007/BF00655002 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 130 1987 1-2 02 243-254 |
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10.1007/BF00655002 doi (DE-627)OLC2066164593 (DE-He213)BF00655002-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Snijders, M. A. J. verfasserin aut Multi-frequency observations of the 1985 outburst of RS ophiuchi 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract The 1985 outburst of the bright, recurrent nova RS Oph was almost simultaneously observed at X-ray, UV, optical, IR and radio frequencies at many epochs. The abundances in the ejected shell and the development of the bolometric luminosity as a function of time suggest that the cause of the outburst is a nuclear runaway on a massive white dwarf. Radio Frequency White Dwarf Bolometric Luminosity Massive White Dwarf Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 130(1987), 1-2 vom: Feb., Seite 243-254 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:130 year:1987 number:1-2 month:02 pages:243-254 https://doi.org/10.1007/BF00655002 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 130 1987 1-2 02 243-254 |
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Abstract The 1985 outburst of the bright, recurrent nova RS Oph was almost simultaneously observed at X-ray, UV, optical, IR and radio frequencies at many epochs. The abundances in the ejected shell and the development of the bolometric luminosity as a function of time suggest that the cause of the outburst is a nuclear runaway on a massive white dwarf. © D. Reidel Publishing Company 1987 |
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Abstract The 1985 outburst of the bright, recurrent nova RS Oph was almost simultaneously observed at X-ray, UV, optical, IR and radio frequencies at many epochs. The abundances in the ejected shell and the development of the bolometric luminosity as a function of time suggest that the cause of the outburst is a nuclear runaway on a massive white dwarf. © D. Reidel Publishing Company 1987 |
abstract_unstemmed |
Abstract The 1985 outburst of the bright, recurrent nova RS Oph was almost simultaneously observed at X-ray, UV, optical, IR and radio frequencies at many epochs. The abundances in the ejected shell and the development of the bolometric luminosity as a function of time suggest that the cause of the outburst is a nuclear runaway on a massive white dwarf. © D. Reidel Publishing Company 1987 |
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