Physics
Scientific paper
Aug 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phyu...41..807g&link_type=abstract
Physics Uspekhi, Volume 41, Issue 8, pp. 807-814 (1998).
Physics
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 λ 4686 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) solarcycle-like activity periodicity of the star EV Lac, whose mass is only 0.3 solar masses. 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.
No associations
LandOfFree
PHYSICS OF OUR DAYS: 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 PHYSICS OF OUR DAYS: 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 PHYSICS OF OUR DAYS: Flaring red dwarf stars: news from Crimea will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1538430