Evolution of Accretion and X-Rays in Lynds 1228

Details Evolution of Accretion and X-Rays in Lynds 1228 Evolution of Accretion and X-Rays in Lynds 1228

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cxo..prop.2103g&link_type=abstract

Chandra Proposal ID #08200495

Computer Science

Chandra Proposal Id #08200495

Scientific paper

We propose to observe two centers of low-mass star formation in the Lynds 1228 dark cloud. L1228 is one of the most active star-formation regions within the Cepheus giant molecular cloud complex. Recent Spitzer Space Telescope observations have shown a wide variety of pre-main sequence stars at various stages of evolution, ranging from embedded, jet+outflow driving protostars to classical and weak-lined T Tauri stars with very different circumstellar-disk characteristics. We aim at studying the influence of accretion and disk parameters on X-ray production in a region with characteristics intermediate between the Taurus and the Orion star-forming regions.

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