Ultraviolet studies of stars in the populous cluster NGC 2100 in the Large Magellanic Cloud

Details Ultraviolet studies of stars in the populous cluster NGC 2100 in the Large Magellanic Cloud Ultraviolet studies of stars in the populous cluster NGC 2100 in the Large Magellanic Cloud

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...292..130b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 292, May 1, 1985, p. 130-142.

Astronomy and Astrophysics

Astronomy

16

B Stars, Galactic Clusters, Magellanic Clouds, O Stars, Stellar Spectrophotometry, Ultraviolet Astronomy, Color-Magnitude Diagram, Interstellar Extinction, Spectral Energy Distribution, Stellar Temperature, Supergiant Stars

Scientific paper

The authors have studied the ultraviolet energy distributions of the B stars in the LMC cluster NGC 2100. The ultraviolet extinction law was studied for the LMC cluster. The Teff-luminosity diagrams were determined. The brightest stars in the clusters are evolved stars on the "horizontal" supergiant branch. No P Cygni profiles indicating mass loss were recognized for these supergiants.

Affiliated with

Also associated with

No associations

Rating

Ultraviolet studies of stars in the populous cluster NGC 2100 in the Large Magellanic Cloud 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 Ultraviolet studies of stars in the populous cluster NGC 2100 in the Large Magellanic Cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet studies of stars in the populous cluster NGC 2100 in the Large Magellanic Cloud will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1631126