Molecular Hydrogen in the Circumstellar Environment of Herbig Ae/Be Stars

Details Molecular Hydrogen in the Circumstellar Environment of Herbig Ae/Be Stars Molecular Hydrogen in the Circumstellar Environment of Herbig Ae/Be Stars

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..348..291m&link_type=abstract

Astrophysics in the Far Ultraviolet: Five Years of Discovery with FUSE ASP Conference Series, Vol. 348, Proceedings of the Confe

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We present our analysis of the molecular hydrogen in the circumstellar environment of a sample of Herbig Ae/Be stars observed with FUSE. The characteristics of H2 around Herbig Ae and Be stars gives evidence of two mechanisms of excitation. This suggests structural differences between Herbig Ae and Be stars' environments which could be explained by a faster evolution of the latter combined with stronger radiation fields.

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