X-ray emission as a tracer of circumstellar matter around herbig ae/be stars

Details X-ray emission as a tracer of circumstellar matter around herbig ae/be stars X-ray emission as a tracer of circumstellar matter around herbig ae/be stars

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..587z&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 587-588

Astronomy and Astrophysics

Astrophysics

4

Stars: Herbig Ae/Be

Scientific paper

We have detected X-ray emission (1 keV) from young intermediate-mass stars (Herbig Ae/Be stars). Since these stars are not supposed to produce intrinsic X-ray emission (no convection, no coronae), we believe that our results suggest that the X-ray emission actually traces the shock interaction of the Ae/Be star stellar winds with remnant circumstellar matter left over from the star formation process, the presence of which is also indicated by far-infrared (IRAS) and submm/mm continuum data.

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