Multi-Wavelength Signatures of Magnetic Activity in the Star-Forming Region around LkHa101

Details Multi-Wavelength Signatures of Magnetic Activity in the Star-Forming Region around LkHa101 Multi-Wavelength Signatures of Magnetic Activity in the Star-Forming Region around LkHa101

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1654w&link_type=abstract

Chandra Proposal ID #06200872

Physics

Chandra Proposal Id #06200872

Scientific paper

Among several classes of active stars and solar flares, a tight relation is found between X-ray and radio luminosities. This relation, which implies an intimate physical connection, has been subject to coordinated radio and X-ray studies for particular active binaries and dMe stars, but never among one of the most active classes of stars, pre-main sequence stars. Here, we propose a pair of 40ks coordinated VLA/ACIS-I observations of the nearby young cluster around LkHa101. We will examine the X-ray radio connection simultaneously for several scores of stars. The data will tighten the relation of the quiescent emission and study the causal relation of radio and X-ray flares for young stars with and without disks.

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