Flaring red dwarf stars: news from Crimea.

Details Flaring red dwarf stars: news from Crimea. Flaring red dwarf stars: news from Crimea.

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998svphu..41..807g&link_type=abstract

Soviet Physics Uspekhi, Vol. 41, No. 8, p. 807 - 814

Physics

Variables: Stellar Models, Variables: Starspots, Variables: Red Dwarfs

Scientific paper

Important phenomena are briefly described which have recently been discovered in the Crimean studies of flaring red dwarf stars believed to be the most common type of variable stars in the Galaxy. These phenomena include (i) long-lived radiation from a blueshifted component in the ionized-helium λ4686 Å emission line in the active state of one such star, (ii) a long-lived absorption component in the stellar flare light curves with a lifetime exceeding that of the conventional flare emission, and (iii) solar cycle-like activity periodicity of the star EV Lac, whose mass is only 0.3 Msun. In theoretical terms, a red dwarf star spot model is constructed which, in contrast to the commonly accepted model, agrees well with the solar spot picture.

Affiliated with

Also associated with

No associations

Rating

Flaring red dwarf stars: news from Crimea. 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 Flaring red dwarf stars: news from Crimea., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Flaring red dwarf stars: news from Crimea. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1543432