X-Rays from Stars at the Far End of the Main Sequence

Details X-Rays from Stars at the Far End of the Main Sequence X-Rays from Stars at the Far End of the Main Sequence

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cxo..prop..747g&link_type=abstract

Chandra Proposal ID #03200093

Physics

Chandra Proposal Id #03200093

Scientific paper

ACIS observations and detection of HH2 has shown that these outflows can
generate X-rays when they strike the ISM. To increase the sample, we
propose to search for HH80/81 which should be more luminous but farther
away..

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