Herbig Ae/Be Stars

Details Herbig Ae/Be Stars Herbig Ae/Be Stars

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..355...87w&link_type=abstract

Stars with the B[e] Phenomenon. ASP Conference Series, Vol. 355, Proceedings of the Conference Held 10-16 July, 2005, at the Isl

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Herbig Ae/Be stars are intermediate mass pre-main-sequence stars surrounded by remnants of the star formation process. These remnants include a passive, gas-rich and dusty proto-planetary disk and loosely bound material from the parent molecular cloud. The composition and geometry of the circumstellar material is discussed, as well as evidence for planet formation.

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