Cyclicity in the variability of R Coronae Borealis

Details Cyclicity in the variability of R Coronae Borealis Cyclicity in the variability of R Coronae Borealis

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997kfnt...13d..82r&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 13, p. 82

Astronomy and Astrophysics

Astronomy

Variable Stars, Stellar Coronas, Light Curve, Angular Velocity, Stellar Spectra, Astronomical Photometry, Diurnal Variations, Stellar Luminosity

Scientific paper

A simple analysis of the visual light curve of R CrB since 1843 has
revealed a 4400 +/- 400-day cycle in the sequence of visual light
minima. It has settled since the thirties of this century. Minima in the
second half of the cycle occur less frequently and are shallower. This
cyclicity may be due to variations of mass loss rate of the star.

Affiliated with

Also associated with

No associations

Rating

Cyclicity in the variability of R Coronae Borealis 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 Cyclicity in the variability of R Coronae Borealis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cyclicity in the variability of R Coronae Borealis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-806779