Magnetic Heating of the Outer Atmospheres of Very Low Mass Dwarfs

Details Magnetic Heating of the Outer Atmospheres of Very Low Mass Dwarfs Magnetic Heating of the Outer Atmospheres of Very Low Mass Dwarfs

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop12011o&link_type=abstract

HST Proposal ID #12011. Cycle 17

Computer Science

Scientific paper

The detections of FUV and X-ray emissions from very low mass stars and browndwarfs have confirmed that stellar magnetic activity can survive even at theselow stellar masses. The emissions are qualitatively similar to those from activestars, despite the dramatic differences between the characteristics of It iscurrently an open question how the structures and magnetic heating which existsin these very low mass stars compare with those seen in higher mass active stars.We propose to take Chandra and HST/COS spectra of two nearby active very lowmass stars in order to determine the effect that these large-scale fields have ontransition region and coronal structures.;

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