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Multiwavelength studies of five chromospherically active stars

Show simple item record Pandey, J. C. Singh, K. P. Sagar, R. Drake, S. A. 2009-07-02T09:13:24Z 2009-07-02T09:13:24Z 2007
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

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