X-Rays from the Nearest Protostars: L1551

Details X-Rays from the Nearest Protostars: L1551 X-Rays from the Nearest Protostars: L1551

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..542b&link_type=abstract

Chandra Proposal ID #02200178

Astronomy and Astrophysics

Astrophysics

Chandra Proposal Id #02200178

Scientific paper

The discovery of hard X-ray emission from protostars may have profound implications for the astrophysics of star formation the earliest phases of stellar evolution. The Lynds 1551 cloud in the Taurus-Auriga complex is the closest group of actively forming stars with several Class 0/I protostars and outflows lying in a single ACIS-I field. The proposed observation will give an extremely sensitive measurements of these protostars and other young stars, and will search for X-rays emission from Herbig-Haro shocks.

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