The Age-Rotation Relation in Late-Type Stars Between ~1-10 MYR

Details The Age-Rotation Relation in Late-Type Stars Between ~1-10 MYR The Age-Rotation Relation in Late-Type Stars Between ~1-10 MYR

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cxo..prop..756s&link_type=abstract

Chandra Proposal ID #03200289

Physics

Chandra Proposal Id #03200289

Scientific paper

We propose to conduct a fundamental census of X-ray emission from stars in Orion and NGC 2264 for which we have a wealth of supporting multi-wavelength data. This will allow us to investigate a wide variety of scientific questions. The most important scientific goal of this study is investigating the relationship between age, rotation, and X-ray activity for late-type stars ranging in age from ~1-10 Myr. Understanding the X-ray environment of young stars and how rotation is related to X-ray flux has direct implications for the chemical and dynamical evolution of protoplanetary disks, and, consequently, for planet formation.

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