On the nature of M28 V7

Details On the nature of M28 V7 On the nature of M28 V7

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97..962m&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Oct. 1985, p. 962-965.

Astronomy and Astrophysics

Astronomy

4

Cataclysmic Variables, Globular Clusters, Variable Stars, Binary Stars, Mira Variables, Stellar Spectra

Scientific paper

It has recently been suggested that V7 in NGC 6626 (M28) may be one of the few known cataclysmic variables in a globular cluster. The authors have obtained the spectrum of the object, and find it instead to be near type M5 III, and thus probably a normal Mira variable. However, if V7 is indeed a member of the cluster (which is far from certain), then it proves to be very interesting for an entirely different reason: it would represent the first high-amplitude Mira variable in a moderately metal-poor cluster.

Affiliated with

Also associated with

No associations

Rating

On the nature of M28 V7 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 On the nature of M28 V7, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the nature of M28 V7 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1547802