CCD photometry of late-type stars in the young open cluster IC 2602

Details CCD photometry of late-type stars in the young open cluster IC 2602 CCD photometry of late-type stars in the young open cluster IC 2602

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26as..126...81f&link_type=abstract

A & A Supplement series, Vol. 126, November II 1997, 81-90.

Astronomy and Astrophysics

Astronomy

4

Stars: Evolution, Stars: Late-Type, Open Clusters: Individual, Ic 2602

Scientific paper

We present the results of VRI photometry of the young open cluster IC 2602. Two 15 arcmin times 15 arcmin fields were observed in February and May 1991 using the 1-m Swope telescope at Las Campanas. Using theoretical isochrones obtained from \cite[D'Antona & Mazzitelli (1994)]{dam94}, and allowing for observational and other uncertainties, we identify 78 primary candidate members with 12= 50%, as might be expected given its low galactic latitude. We also compare our photometry with that given for the X-ray detected stars of \cite[Randich et al. (1995)]{ran95}. We present complimentary narrow band H alpha photometry for a subset of the stars.

Affiliated with

Also associated with

No associations

Rating

CCD photometry of late-type stars in the young open cluster IC 2602 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 CCD photometry of late-type stars in the young open cluster IC 2602, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CCD photometry of late-type stars in the young open cluster IC 2602 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1683470