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Paper: Massive Pre-Main Sequence Stars in the Young Open Cluster NGC 1893
Volume: 267, Hot Star Workshop III: the Earliest Stages of Massive Star Birth
Page: 389
Authors: Marco, A.; Negueruela, I.; Steele, I. A.
Abstract: 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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