Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988japa....9..107r&link_type=abstract
Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 9, June 1988, p. 107-116.
Astronomy and Astrophysics
Astrophysics
5
B Stars, Binary Stars, Interstellar Extinction, Peculiar Stars, Stellar Color, Stellar Rotation, Angular Velocity, H Beta Line, Star Clusters, Stellar Magnitude
Scientific paper
Analysis of the available observational data for the Alpha-Persei cluster members shows that rotation effects on the intermediate-band indices c1 and (u-b) are considerable. In c1, rotation produces a reddening of 0.040 magnitudes per 100 km/s. In (u-b), the effect for B stars is found to be 0.06 magnitudes per 100 km/s of V sin i. The binaries and peculiar stars are found to behave differently in the color excess (due to rotation) versus V sin i diagrams. These empirical effects can be utilized to recalibrate these color indices and also to separate members that are either chemically peculiar or in binary systems.
Mathew Annamma
Rajamohan R.
No associations
LandOfFree
Effects of rotation on the colours and line indices of stars. I - The Alpha Persei Cluster 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 Effects of rotation on the colours and line indices of stars. I - The Alpha Persei Cluster, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effects of rotation on the colours and line indices of stars. I - The Alpha Persei Cluster will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1181716