Spectroscopic and photometric properties of red stars in the bar of the Large Magellanic Cloud

Details Spectroscopic and photometric properties of red stars in the bar of the Large Magellanic Cloud Spectroscopic and photometric properties of red stars in the bar of the Large Magellanic Cloud

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..310..340l&link_type=abstract

Variable Stars in the Local Group, IAU Colloquium 193, Proceedings of the conference held 6-11 July, 2003 at Christchurch, New Z

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Spectroscopy and variability studies of red stars in the Bar of the LMC enable the stars to be classed as spectral type M, S or C and as variables of class L, SR, or Mira. The reults are compared with the data for Magellanic Cloud star clusters and for the galactic field. The number of S stars relative to carbon stars in generally high in comparison to theoretical expectation.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic and photometric properties of red stars in the bar of 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 Spectroscopic and photometric properties of red stars in the bar of the Large Magellanic Cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic and photometric properties of red stars in the bar of the Large Magellanic Cloud will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1056411