Young Stars and Outflows in LYNDS 1641

Details Young Stars and Outflows in LYNDS 1641 Young Stars and Outflows in LYNDS 1641

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..219g&link_type=abstract

Chandra Proposal ID #01200050

Physics

Chandra Proposal Id #01200050

Scientific paper

The Orion molecular cloud contains a wide range of star forming environments, from rich high-mass clusters to distributed low-mass star formation. This observation focuses on the latter. The field includes a number of T Tauri stars, the Herbig Ae/Be star V380, and the high-velocity Herbig-Haro objects HH-1 and HH-2. Soft X-rays from the outflow, or hard Fe-K emission from a diffuse plasma, may also be detected. A short exposure will resolve the whether the B9 star HD 37001 or a nearby M4 star is responsible for the ROSAT source RX0535-0633.

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