Multiwavelength studies of five chromospherically active stars

Pandey, J. C. ; Singh, K. P. ; Sagar, R. ; Drake, S. A. (2007) Multiwavelength studies of five chromospherically active stars Proceedings of the conference held 1-5 November, 2005 in Sejong University . pp. 74-79.

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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.

Item Type:Article
Source:Copyright of this article belongs to ASP Conference Series.
ID Code:91687
Deposited On:23 May 2012 14:13
Last Modified:12 Jul 2012 05:12

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