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Flare Stars in Star Clusters, Associations and the Solar Vicinity - Proceedings of the 137th Symposium of the International Astronomical Union Held in Byurakan (Armenia), U.S.S.R., October 23-27, 1989 (Paperback, Softcover reprint of the original 1st ed. 1990)
Loot Price: R3,049
Discovery Miles 30 490
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Flare Stars in Star Clusters, Associations and the Solar Vicinity - Proceedings of the 137th Symposium of the International Astronomical Union Held in Byurakan (Armenia), U.S.S.R., October 23-27, 1989 (Paperback, Softcover reprint of the original 1st ed. 1990)
Series: International Astronomical Union Symposia, 137
Expected to ship within 10 - 15 working days
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Stellar flares represent one of the most challenging problems of
contemporary astrophysics. Both solar and stellar observations have
shown the flare phenomenon to be very complex, and in recent years
important progress has been made from simultaneous observations
over wide wavelength ranges. Some similarities exist between solar
and stellar flares, but im portant differences have also been
established. Such topics, as well as theoretical aspects, were
discussed in detail at the Palo Alto IAU Colloquium No. 104, Solar
and Stellar Flares, in 1988. Another approach to the study of
stellar flares is through observations of flare stars in physical
systems. The possibility of detecting flare stars in star clusters
and associations with wide angle telescopes have allowed
observations of systems with quite different ages. The classical
works of G. Haro and V. A. Ambartsumian demonstrated the
evolutionary nature of the flare phenomenon. Flares occur at the
earliest stages of dwarf star evolution. The photographic
observations of flare stars in systems of different ages turned out
to be significant not only for the evolutionary study of flare
stars, but also for the study of their physical nature. This
observational fact was conditioned by very large diversity of flare
star luminosities, i.e. of scales of flares produced by them and by
peculiarities of stellar flares observed in star clusters and
associations."
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