A Chandra Study of Herbig-Haro Objects: HH184 & HH300

Details A Chandra Study of Herbig-Haro Objects: HH184 & HH300 A Chandra Study of Herbig-Haro Objects: HH184 & HH300

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.7428p&link_type=abstract

American Astronomical Society Meeting 207, #74.28; Bulletin of the American Astronomical Society, Vol. 37, p.1289

Astronomy and Astrophysics

Astronomy

Scientific paper

Recent data obtained by the Chandra X-ray Observatory has demonstrated that the jet launch and collimation region of protostellar jets contain high-temperature X-ray emitting plasma; a previously unknown property from low frequency studies. Thus, providing evidence that protostellar jets could possibly be considered as strong X-ray emitters. Here, we present Chandra observations of Herbig-Haro objects HH184 and HH300, and explore the possible origin of their X-ray emission: unabsorbed jet emission from HH184 versus protostellar emission from HH300.

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