Massive Pre-Main Sequence Stars in the Young Open Cluster NGC 1893

Details Massive Pre-Main Sequence Stars in the Young Open Cluster NGC 1893 Massive Pre-Main Sequence Stars in the Young Open Cluster NGC 1893

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..267..389m&link_type=abstract

Hot Star Workshop III: The Earliest Stages of Massive Star Birth. ASP Conference Proceedings, Vol. 267. Edited by Paul A. Crowth

Astronomy and Astrophysics

Astronomy

Scientific paper

We have identified a population of massive pre-main sequence (PMS) stars in the young open cluster NGC 1893. The presence of Herbig AeBe stars in the vicinity of O-type stars likely to be a few Myr old and their co-existence with B-type main sequence objects of later spectral types indicate that massive star formation is still ongoing in NGC 1893 and has been taking place over a relatively long timescale.

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