Photometry of the unique luminous red variable in M31

Details Photometry of the unique luminous red variable in M31 Photometry of the unique luminous red variable in M31

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasp..104..179b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 104, March 1992, p. 179-181. Research supported by NASA

Astronomy and Astrophysics

Astronomy

16

Andromeda Galaxy, Astronomical Photometry, Novae, Variable Stars, Galactic Bulge, Light Curve, Luminosity

Scientific paper

Additional photometric observations of an unusual red nova that appeared in M31 in 1988 are presented. It was shown by means of mV observations that the nova is a very red object, in agreement with observations presented by Rich et al. (1989) and Mould et al. (1990). The nova was found to fall well off the maximum magnitude versus rate of decline relationship shown in Rosino (1964) and van den Bergh (1988).

Affiliated with

Also associated with

No associations

Rating

Photometry of the unique luminous red variable in M31 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 Photometry of the unique luminous red variable in M31, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometry of the unique luminous red variable in M31 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1490568