CCD photometry of galactic clusters containing Cepheid variables. II - NGC 6067

Details CCD photometry of galactic clusters containing Cepheid variables. II - NGC 6067 CCD photometry of galactic clusters containing Cepheid variables. II - NGC 6067

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214...45w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, May 1, 1985, p. 45-53.

Astronomy and Astrophysics

Astronomy

22

Astronomical Photometry, Cepheid Variables, Charge Coupled Devices, Color-Magnitude Diagram, Galactic Clusters, Open Clusters, Star Distribution

Scientific paper

A colour-magnitude diagram extending to V = 19 is given for 1019 stars in the open cluster NGC 6067. The true distance modulus is found to be 11.05±0.10 mag assuming E(B-V) = 0.35. A colour-magnitude diagram for an adjacent field shows that the Norma star cloud is at a similar distance to NGC 6067. The Cepheids CPD -53°7400A (p = 11.3 day) and HD 144972 (p = 3.8 day) have >MV< = -3.77±0.10 and >MV< = -3.27±0.10, respectively, if they are cluster members.

Affiliated with

Also associated with

No associations

Rating

CCD photometry of galactic clusters containing Cepheid variables. II - NGC 6067 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 galactic clusters containing Cepheid variables. II - NGC 6067, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CCD photometry of galactic clusters containing Cepheid variables. II - NGC 6067 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1632856