Activity cycles in solar-type stars

Details Activity cycles in solar-type stars Activity cycles in solar-type stars

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...73r&link_type=abstract

XMM-Newton Proposal ID #04018805

Other

Stars, White Dwarfs, Solar System, Hd 81809, 61 Cyg, Xmm-Newton Proposal 04018805

Scientific paper

We propose to continue the ongoing long-term monitoring program of a sample of solar-type stars to search for cyclic behavior, analogous to the one observed for the Sun, in their X-ray emission. These stars have moderate levels of activity and are thus true ``solar analogs''. XMM-Newton makes it possible, for the first time, to efficiently monitor the low-activity, cyclic stars and to effectively study the characteristics of the activity cycles on stars other than the Sun.

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