The End of Stellar Coronae?

Details The End of Stellar Coronae? The End of Stellar Coronae?

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop...98b&link_type=abstract

Chandra Proposal ID #01200574

Physics

Chandra Proposal Id #01200574

Scientific paper

Almost all stars are X-ray emitters. Convective stars are thought to have analogs of the solar corona, caused by magnetic activity which in turn is produced by a dynamo. There are reasons to believe that the dynamo and coronal heating could change character near the bottom of the main sequence. We get to the heart of this by going to the very bottom of the main sequence, and below to the brown dwarf regime. We test 2 of the nearest known such objects to see if they lie beyond the end of the realm of stellar coronae.

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