A Spectroscopic Survey of NGC 7419

Details A Spectroscopic Survey of NGC 7419 A Spectroscopic Survey of NGC 7419

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361..472n&link_type=abstract

Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere

Physics

1

Scientific paper

The reddened open cluster NGC7419 is believed to have a very high fraction of Be stars and present an exceptionally high number of red supergiants (five for no blue supergiants). We present the first results of our recent spectroscopic observations of the cluster, which confirm the high fraction of Be stars. We also find spectral types in good agreement with a location in the Perseus Arm.

Affiliated with

Also associated with

No associations

Rating

A Spectroscopic Survey of NGC 7419 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A Spectroscopic Survey of NGC 7419, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Spectroscopic Survey of NGC 7419 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-858119