Emission from Late-Type Star AD Leo

Details Emission from Late-Type Star AD Leo Emission from Late-Type Star AD Leo

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..442m&link_type=abstract

Chandra Proposal ID #02200080

Physics

Chandra Proposal Id #02200080

Scientific paper

Our proposed program to understand the x-ray emission from late-type stars will address three important issues: i) establish whether the "solar analogy" is invariably appropriate (and under what circumstance it may not apply), ii) determine coronal characteristics and their dependence on the properties of the underlaying stars (including rotations, color, and metallicity), and iii) understand the variation of activity levels at the low-mass end of the main sequence, where the convection zone may penetrate to near the stellar center.

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