VI photometry of Berkeley 66 (Guarnieri+ 1997)

Details VI photometry of Berkeley 66 (Guarnieri+ 1997) VI photometry of Berkeley 66 (Guarnieri+ 1997)

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..41210451g&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/121/451. Originally published in: 1997A&AS..121..451G

Computer Science

Clusters: Open, Photometry

Scientific paper

A colour magnitude diagram (CMD) extending to V=~19mag is given for 444 stars in the region of the galactic cluster Berkeley 66. The V and I photometry of a nearby field is also reported. This object appears very faint, highly contaminated by foreground stars and very reddened. The apparent distance modulus (m-M) and the colour excess EV-I are guessed to be 17.5 and 1.1, respectively, with an uncertainty of at least 30%. Adopting these values the comparison of the CMD with theoretical isochrones from the Padova group provides an age around 1.0Gyr. (1 data file).

Affiliated with

Also associated with

No associations

Rating

VI photometry of Berkeley 66 (Guarnieri+ 1997) 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 VI photometry of Berkeley 66 (Guarnieri+ 1997), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VI photometry of Berkeley 66 (Guarnieri+ 1997) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1305362