The outer atmospheres of flare stars discovered with GALEX in the near-UV

Details The outer atmospheres of flare stars discovered with GALEX in the near-UV The outer atmospheres of flare stars discovered with GALEX in the near-UV

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop..131s&link_type=abstract

XMM-Newton Proposal ID #06536810

Computer Science

Stars, White Dwarfs, Solar System, Source 4, Source 7, Source 17, Source 18, Source 32, Source 45

Scientific paper

Magnetic activity produces copious UV and X-ray emission in the chromosphere, transition region and corona of late-type stars. Both types of radiation are believed to be crucial for the evolution of the atmospheres of the planet but their relative importance is not known. While X-rays penetrate deeper into the planet atmosphere, UV fluxes may be higher and significantly affect the outer layers of the planet atmosphere. We aim at a comprehensive study of the strength and range of X-ray and UV fluxes for M dwarfs identified in the GALEX All-Sky Survey. In this proposal we ask for the corresponding X-ray measurements.

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