Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26as...29...15c&link_type=abstract
Astronomy and Astrophysics Supplement Series, vol. 29, July 1977, p. 15-30. Research supported by the Universidad Catolica de C
Astronomy and Astrophysics
Astrophysics
21
Late Stars, M Stars, Mira Variables, Ubv Spectra, Variable Stars, Graphs (Charts), Light Curve, Stellar Spectrophotometry, Tables (Data)
Scientific paper
A total of 3743 V, B-V and U-B photoelectric measurements of 60 Mira-type variable stars, mainly in the southern hemisphere, were made at the Cerro Tololo Inter-American Observatory during 14 observation periods, from December 1972 to March 1974. Light curves are given for each star based on a probable graphic interpolation as a function of time. Elements of each light and color curve are derived. The principal characteristics observed in the V curves are that the form of variation remains the same in each star and that there are groups of stars whose light curves are similar, even though the elements are not constant. The variation of the color indices is also analyzed, showing the most important properties.
No associations
LandOfFree
Light and colour variation of the Mira 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 Light and colour variation of the Mira stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Light and colour variation of the Mira stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1559369