Empirical light curve of a star with the R Coronae Borealis phenomenon

Details Empirical light curve of a star with the R Coronae Borealis phenomenon Empirical light curve of a star with the R Coronae Borealis phenomenon

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18...65r&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 65; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 2, Feb. 1992, p. 158-

Astronomy and Astrophysics

Astronomy

3

Light Curve, R Coronae Borealis Stars, Stellar Luminosity, Stellar Models, Stellar Spectrophotometry, Variability

Scientific paper

The application of an empirical formula to describe the photometric behavior of stars with the R Coronae Borealis (RCB) phenomenon, i.e., stars which exhibit the formation and ejection of the dust layer, shows the prospects of this approach, which makes it possible to obtain some standard pattern for this phenomenon and, consequently, facilitate its theoretical interpretation. The presence of a unified description of the process of the formation and ejection of the dust layer points to the significance of the initial conditions, which determine the entire subsequent development of a phenomenon of the RCB type.

Affiliated with

Also associated with

No associations

Rating

Empirical light curve of a star with the R Coronae Borealis phenomenon 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 Empirical light curve of a star with the R Coronae Borealis phenomenon, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Empirical light curve of a star with the R Coronae Borealis phenomenon will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1052619