Optical Spectroscopy of the nova-like variable V 445 Puppis

dc.contributor.author	Kamath, U. S
dc.contributor.author	Anupama, G. C
dc.date.accessioned	2008-07-22T06:11:37Z
dc.date.available	2008-07-22T06:11:37Z
dc.date.issued	2002-09
dc.identifier.citation	BASI, Vol. 30, No. 3, pp. 679 - 681	en
dc.identifier.uri	http://hdl.handle.net/2248/2790
dc.description.abstract	V445 Puppis is a peculiar variable which had a nova-like eruption in December 2000. The early spectra did not show any emission lines of hydrogen or helium. Fe II lines were very dominant during this phase. We present optical spectra of the early-decline phase of V 445 Pup obtained from the Vainu Bappu Observatory during Feb-April 2001.	en
dc.format.extent	83695 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Stars-Variable-Nova-like	en
dc.subject	Spectroscopy-Optical	en
dc.subject	Stars-Individual-V445 Puppis	en
dc.title	Optical Spectroscopy of the nova-like variable V 445 Puppis	en
dc.type	Article	en