Periodicities in the flare star H II 2411

Details Periodicities in the flare star H II 2411 Periodicities in the flare star H II 2411

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991rmxaa..22..213c&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica (ISSN 0185-1101), vol. 22, Oct. 1991, p. 213-215. Research supported by COSNET-SEP

Astronomy and Astrophysics

Astronomy

1

Flare Stars, Periodic Variations, Stellar Flares, Stellar Luminosity

Scientific paper

The repetitions of the flare star H II 2411 are analyzed to determine whether periodicities exist in the flare phenomena. The data are taken from observations beginning in 1962 and are subjected to analysis by the formalism by Lomb (1976) and Scargle (1982) which accounts for both nonuniform point-spacing and observational noise. Two periods are identified, and the flare phenomena in the object are found to be similar to the flare activities of the sun.

Affiliated with

Also associated with

No associations

Rating

Periodicities in the flare star H II 2411 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 Periodicities in the flare star H II 2411, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Periodicities in the flare star H II 2411 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1877031