Multiwavelength studies of five chromospherically
active stars

dc.contributor.author	Pandey, J. C.
dc.contributor.author	Singh, K. P.
dc.contributor.author	Sagar, R.
dc.contributor.author	Drake, S. A.
dc.date.accessioned	2009-07-02T09:13:24Z
dc.date.available	2009-07-02T09:13:24Z
dc.date.issued	2007
dc.identifier.uri	http://hdl.handle.net/123456789/102
dc.description.abstract	We present a multiwavelength study of five chromospherically active stars, including newly obtained optical photometry, low-resolution optical spectroscopy, as well as archival X-ray observations. The bulk of the optical, X- ray, and kinematical data indicate that the stars FR Cnc, HD 95559, HD 160934 and LO Peg are all active, young stars of 100 Myrs or less, whose activity levels are primarily due to their youth. All the photometric, spectroscopic and X-ray observations suggest that the star HD 81032 is a newly identified, evolved RS CVn-type binary.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	asp362-74
dc.subject	Active Stars, Ray Flares	en_US
dc.title	Multiwavelength studies of five chromospherically active stars	en_US
dc.type	Article	en_US