Computer Science
Scientific paper
Jul 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sfet.confe..30g&link_type=abstract
"Star Formation in the Era of Three Great Observatories, meeting abstracts from the conference held July 13-15, 2005 in Cambridg
Computer Science
Scientific paper
Since most stars in the Galaxy probably formed in giant molecular clouds, identifying nearly complete samples of low-mass stars in galactic star-forming regions is an important step in understanding the overall star-formation process. Recent X-ray, optical, and near-infrared studies of the galactic HII regions M8, M16, M17 and M20 have significantly increased the number of known cluster stars. By comparing their X-ray and infrared properties with stars in well-studied regions like the Orion Nebula Cluster, we can estimate distance, age and completeness. These studies will be used to assess the prevalence of triggered star-formation.
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