High speed photometry of PG 1012-029

dc.contributor.author	Ashoka, B. N
dc.contributor.author	Seetha, S
dc.contributor.author	Marar, T. M. K
dc.contributor.author	Kasturirangan, K
dc.contributor.author	Rao, U. R
dc.contributor.author	Bhattacharyya, J. C
dc.date.accessioned	2008-07-14T08:58:00Z
dc.date.available	2008-07-14T08:58:00Z
dc.date.issued	1994-03
dc.identifier.citation	Astronomy and Astrophysics, Vol. 283, No. 2, pp. 455 - 462	en
dc.identifier.issn	0004-6361
dc.identifier.uri	http://hdl.handle.net/2248/2671
dc.description.abstract	High speed optical photometric observations of PG 1012 - 029, conducted during 1990-1991, confirm the nova-like classification of the object. Several eclipses observed by us have been used to refine the orbital period of the system. Variations in the light curves and in particular, the presence of a bright hot spot in our 1991 data are high-lighted. We also deduce a maximum mass transfer rate of 1.5 10-8 solar mass/yr for the system.	en
dc.format.extent	928620 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	European Southern Observatory	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1994A%26A...283..455A	en
dc.subject	Accretion Disks	en
dc.subject	Brightness	en
dc.subject	Cataclysmic Variables	en
dc.subject	Computational Astrophysics	en
dc.subject	Eclipsing Binary Stars	en
dc.subject	Stellar Mass	en
dc.subject	Astronomical Photometry	en
dc.subject	High Speed	en
dc.subject	Light Curve	en
dc.subject	Mass Transfer	en
dc.subject	Stellar Orbits	en
dc.title	High speed photometry of PG 1012-029	en
dc.type	Article	en