Pascal and Francis Bibliographic Databases

Help

Permanent link : http://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=21900992

Export

Selection :

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
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

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

Access to the document

Searching the Web