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Time Evolution Of X-Ray Coronal Activity In Pms Stars; A Possible Relation With The Evolution Of Accretion Disks

ASTRONOMY & ASTROPHYSICS, no. 1 (2003): 277-292

Cited: 97|Views24

Abstract

We investigate the evolution of X-ray stellar activity from the age of the youngest known star forming regions (SFR), less than or similar to 1 Myr, to about 100 Myr, i.e. the zero age main sequence (ZAMS) for a similar to 1 M. star. We consider five SFR of varying age (rho Ophiuchi, the Orion Nebula Cluster, NGC 2264, Chamaeleon I, and e...More

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