A 2.09-h Photometric Periodicity in GW Librae
Abstract We have found a 2.09 h modulation in brightness of the dwarf nova GW Lib. This bears no special relationship to the 1.28 h spectroscopic period that is believed to be the orbital period. It was present in May 2001, but not in observations made in 1997 and 1998 and is of unknown origin. Simi...
Ausführliche Beschreibung
Autor*in: |
Woudt, Patrick A. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
2002 |
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Schlagwörter: |
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Anmerkung: |
© Kluwer Academic Publishers 2002 |
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Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 282(2002), 2 vom: Okt., Seite 433-438 |
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Übergeordnetes Werk: |
volume:282 ; year:2002 ; number:2 ; month:10 ; pages:433-438 |
Links: |
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DOI / URN: |
10.1023/A:1020809407912 |
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Katalog-ID: |
OLC2066234249 |
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10.1023/A:1020809407912 doi (DE-627)OLC2066234249 (DE-He213)A:1020809407912-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Woudt, Patrick A. verfasserin aut A 2.09-h Photometric Periodicity in GW Librae 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2002 Abstract We have found a 2.09 h modulation in brightness of the dwarf nova GW Lib. This bears no special relationship to the 1.28 h spectroscopic period that is believed to be the orbital period. It was present in May 2001, but not in observations made in 1997 and 1998 and is of unknown origin. Similar unexplained periodicities are present in FS Aur and V2051 Oph. Orbital Period Light Curve White Dwarf Brightness Modulation Dwarf Nova Warner, Brian aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 282(2002), 2 vom: Okt., Seite 433-438 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:282 year:2002 number:2 month:10 pages:433-438 https://doi.org/10.1023/A:1020809407912 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_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 282 2002 2 10 433-438 |
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10.1023/A:1020809407912 doi (DE-627)OLC2066234249 (DE-He213)A:1020809407912-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Woudt, Patrick A. verfasserin aut A 2.09-h Photometric Periodicity in GW Librae 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2002 Abstract We have found a 2.09 h modulation in brightness of the dwarf nova GW Lib. This bears no special relationship to the 1.28 h spectroscopic period that is believed to be the orbital period. It was present in May 2001, but not in observations made in 1997 and 1998 and is of unknown origin. Similar unexplained periodicities are present in FS Aur and V2051 Oph. Orbital Period Light Curve White Dwarf Brightness Modulation Dwarf Nova Warner, Brian aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 282(2002), 2 vom: Okt., Seite 433-438 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:282 year:2002 number:2 month:10 pages:433-438 https://doi.org/10.1023/A:1020809407912 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_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 282 2002 2 10 433-438 |
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A 2.09-h Photometric Periodicity in GW Librae |
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Abstract We have found a 2.09 h modulation in brightness of the dwarf nova GW Lib. This bears no special relationship to the 1.28 h spectroscopic period that is believed to be the orbital period. It was present in May 2001, but not in observations made in 1997 and 1998 and is of unknown origin. Similar unexplained periodicities are present in FS Aur and V2051 Oph. © Kluwer Academic Publishers 2002 |
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Abstract We have found a 2.09 h modulation in brightness of the dwarf nova GW Lib. This bears no special relationship to the 1.28 h spectroscopic period that is believed to be the orbital period. It was present in May 2001, but not in observations made in 1997 and 1998 and is of unknown origin. Similar unexplained periodicities are present in FS Aur and V2051 Oph. © Kluwer Academic Publishers 2002 |
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Abstract We have found a 2.09 h modulation in brightness of the dwarf nova GW Lib. This bears no special relationship to the 1.28 h spectroscopic period that is believed to be the orbital period. It was present in May 2001, but not in observations made in 1997 and 1998 and is of unknown origin. Similar unexplained periodicities are present in FS Aur and V2051 Oph. © Kluwer Academic Publishers 2002 |
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