B stars in open clusters: fundamental parameters

Details B stars in open clusters: fundamental parameters B stars in open clusters: fundamental parameters

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..276a&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

Stars: Distances, Stars: Emission-Line, Be, Stars: Fundamental Parameters

Scientific paper

We use the BCD spectrophotometric classification system to derive
fundamental parameters of B stars in NGC 2439, NGC 3766 and NGC 6087. We
are able to perform a complete study of each open cluster by deriving
spectral classification of its members, distance modulus and age as
well.

Affiliated with

Also associated with

No associations

Rating

B stars in open clusters: fundamental parameters 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 B stars in open clusters: fundamental parameters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and B stars in open clusters: fundamental parameters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-995276