SAC HD45677 FeII emission lines analysis

Details SAC HD45677 FeII emission lines analysis SAC HD45677 FeII emission lines analysis

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..221m&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

Aurelie observations of the probably Herbig Ae/Be star HD45677 are analysed using the SAC method applied to the various FeII and CrII emission lines components. A comparison with V380 Ori show that FeII lines are opticaly thinner for the object studied. Consequently HD45677 appears to be less evolved than V380 Ori, probably in the phase where the disk is disappearing.

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