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FR Cnc - A Young Spotted Star

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dc.contributor.author Pandey, J. C
dc.date.accessioned 2008-06-05T11:17:56Z
dc.date.available 2008-06-05T11:17:56Z
dc.date.issued 2003
dc.identifier.citation BASI, Vol. 31, No. 3&4, pp. 329 - 331 en
dc.identifier.uri http://hdl.handle.net/2248/2408
dc.description.abstract Optical photometric and spectroscopic studies of the star FR Cnc = BD + 16 1753 have been carried out during the years 2001 - 2002. The star is photometrically variable with a mean period of 0d.8271 ± 0.0002. The rapid changes in the shape of light curve can be attributed to the formation and distribution of two groups of spots on the surface of the star. The presence of strong CaII H, K and H emission lines in the spectra indicates high chromospheric activity in the star. The kinematics of the star suggest that it belongs young population of disk stars. en
dc.format.extent 79731 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.relation.uri http://adsabs.harvard.edu/abs/2003BASI...31..329P en
dc.subject Star en
dc.subject Young en
dc.subject Active en
dc.subject X-ray en
dc.title FR Cnc - A Young Spotted Star en
dc.type Article en


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