UBV Photometry of Known and Potential Variable Stars

Details UBV Photometry of Known and Potential Variable Stars UBV Photometry of Known and Potential Variable Stars

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977javso...5...74k&link_type=abstract

Journal of the American Association of Variable Star Observers, Vol. 5, No. 2, p. 74-75

Physics

3

Variables, Photometry, Ubv Photometry, Ss Cygni

Scientific paper

Standardized UBV photometry of seven early M emission-line dwarfs, seven Mira stars, and also SS Cygni is presented. The dMe stars have not been previously observed in the UBV system to the accuracy presented here. The short time scale ( < 1 min.) variations observed in the light output of SS Cygni are similar to those found by Walker and Chincarini (1968).

Affiliated with

Also associated with

No associations

Rating

UBV Photometry of Known and Potential Variable Stars 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 UBV Photometry of Known and Potential Variable Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UBV Photometry of Known and Potential Variable Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1848049