Plausible explanations for the variations of orbital period in the old nova DQ Herculis
- Author
- DAI, Z. B1 2 3 ; QIAN, S. B1 2
[1] National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, 650011 Kunming, China
[2] United Laboratory of Optical Astronomy, Chinese Academy of Science (ULOAC), 100012 Beijing, China
[3] Graduate School of the CAS, Beijing, China - Source
Astronomy and astrophysics (Berlin. Print). 2009, Vol 503, Num 3, pp 883-888, 6 p ; ref : 3/4 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- cataclysmic variables stars: binaries: eclipsing stars: individual: DQ Herculis stars: novae
- Keyword (fr)
- Binaire éclipse Borne inférieure Cycle solaire Durée trajet Etoile variable cataclysmique Excentricité Naine brune Naine rouge Nova Observation visuelle Orbite circulaire Orbite elliptique Orbite excentrique Transfert masse Variation quasi périodique
- Keyword (en)
- Eclipsing binary stars Lower bound Solar cycle Travel time Cataclysmic variable stars Eccentricity Brown dwarf stars Red dwarf stars Novae Visual observation Circular orbit Elliptic orbit Eccentric orbit Mass transfer Quasi periodic variation
- Keyword (es)
- Cota inferior Observación visual Orbita circular Orbita elíptica Orbita excéntrica Variación semiperiódica
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 21900992
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1051/0004-6361/200810909 
https://dx.doi.org/10.1051/0004-6361/200810909
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