The size of coronae pre-main sequence stars: the eclipsing binary RXJ0529.4+0041

Details The size of coronae pre-main sequence stars: the eclipsing binary RXJ0529.4+0041 The size of coronae pre-main sequence stars: the eclipsing binary RXJ0529.4+0041

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.1886s&link_type=abstract

Chandra Proposal ID #07200307

Physics

Chandra Proposal Id #07200307

Scientific paper

We will derive the size and location of coronal structures of the system RX J0529.4+0041, the first discovered pre-main sequence eclipsing binary with low mass components, through an accurate analysis of the Chandra light curve that will include the primary eclipse and the ingress and egress phases. The determination of the geometry and properties of coronal structures in PMS stars is crucial to understand the physics of their coronae and to study the effects of X-ray emission on the evolution of circumstellar disks, since modification in the ionization rate, chemistry and viscosity, may affect the formation and migration of planets.

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