Integrated Brightness and Colour of Omega-Centauri

Details Integrated Brightness and Colour of Omega-Centauri Integrated Brightness and Colour of Omega-Centauri

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982basi...10..340s&link_type=abstract

Bulletin of the Astronomical Society of India V.10:4, P.340, 1982

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Integrated magnitudes in U, B, V, R and I bands are calculated for the globular cluster Omega Centauri. The observed radial change in the integrated colour of the cluster shows that the cluster core (r < 2arcmin) is redder in R-I colour and bluer in U-B colour. It is argued that there is an increase in the ratio of AGB stars to the red giants towards the centre of the cluster.

Affiliated with

Also associated with

No associations

Rating

Integrated Brightness and Colour of Omega-Centauri 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 Integrated Brightness and Colour of Omega-Centauri, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Integrated Brightness and Colour of Omega-Centauri will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-928863