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Paper: Herbig Ae/Be Stars
Volume: 355, Stars With the B[e] Phenomenon
Page: 87
Authors: Waters, L.B.F.M.
Abstract: 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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