Transition Regions in Very Late M Dwarfs Cycle Later Observations

Details Transition Regions in Very Late M Dwarfs Cycle Later Observations Transition Regions in Very Late M Dwarfs Cycle Later Observations

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5163l&link_type=abstract

HST Proposal ID #5163

Astronomy and Astrophysics

Astrophysics

Hst Proposal Id #5163 Stellar Astrophysics Cool Stars

Scientific paper

We propose to search for transition region emission lines indicative of 1.0E+5 K plasma in the ultraviolet spectra of the coolest M dwarf stars of both the dM and dMe types. With such data we will study the heating rates and energy balance in the transition regions of these stars and compare such data with stars of earlier spectral type. An important question is whether transition regions disappear or have significantly smaller heating rates in the late M dwarfs as is suggested by the X-ray data.

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