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On the Group Formation of Stars in Stellar Associations

Published online by Cambridge University Press:  12 April 2016

L.V. Mirzoyan
L.V. Mirzoyan*
Affiliation:
Byurakan Astrophysical Observatory, Armenia, U.S.S.R.

Extract

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The discovery and study of stellar associations by Ambartsumian (1947, 1954 a) proved two fundamental points regarding the star formation process, e.g., Mirzoyan, 1976. One of them is that the formation process still continues in the present evolution of the Galaxy, and this thesis is not disputed now. According to the second, stars form as physical groups of multiple stars and star clusters, which become stellar associations during the initial phases of their evolution.

Type
Part I: Evolution of Stars in the Post-Main Sequence Stage
Information
International Astronomical Union Colloquium , Volume 69: Binary and Multiple Stars as Tracers of Stellar Evolution , 1982 , pp. 61 - 66
Copyright
Copyright © Reidel 1982

References

Agekian, T.A.: 1954, Astron. Zh, 31, 544.Google Scholar
Allen, C. and Poveda, A.: 1974, The Dynamical Evolution of Trapezium Systems, Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, Mexico, preprint.Google Scholar
Ambartsumian, V.A.: 1937, Astron. Zh. 14, 207.Google Scholar
Ambartsumian, V.A.: 1947, Stellar Evolution and Astrophysics, Ac. Sci. Armenian SSR, Yerevan.Google Scholar
Ambartsumian, V.A.: 1953 a, CR Ac. Sci. Armenian SSR, 16, 73.Google Scholar
Ambartsumian, V.A.: 1953 b, CR Ac. Sci. Armenian SSR, 16, 97.Google Scholar
Ambartsumian, V.A.: 1954 a, Transactions of the IAU, vol. 8, ed. Oosterhoff, P.Th., University Press, Cambridge, p. 665.Google Scholar
Ambartsumian, V.A.: 1954 b, Contr. Byurakan Obs., 15, 3.Google Scholar
Ambartsumian, V.A.: 1956, Vistas in Astronomy, vol. 2, Pergamon Press, London-New York,p. 1708.CrossRefGoogle Scholar
Brutian, G.A.: 1981, private communication.Google Scholar
Markarian, B.E.: 1950, Contr. Byurakan Obs., 5, 3.Google Scholar
Markarian, B.E.: 1951, Contr. Byurakan Obs., 9, 3.Google Scholar
Mirzoyan, L.V.: 1949, CR Ac. Sci. Armenian SSR, 10, 193.Google Scholar
Mirzoyan, L.V.: 1976, in Ambartsumian, V.A. (ed.), Probleme der Modernen Kosmogonie, Birkhäuser Verlag, Basel and Stuttgart, Chapter II.Google Scholar
Mirzoyan, L.V.: 1981, Stellar Nonstability and Evolution, Ac. Sci. Armenian SSR, Yerevan.Google Scholar
Mirzoyan, L.V. and Mnatsakanian, M.A.: 1975, Astrofizika, 11, 551.Google Scholar
Salukvadze, G.N.: 1978, Astrofizika, 14, 57.Google Scholar
Salukvadze, G.N.: 1980a, Astrofizika, 16, 505.Google Scholar
Salukvadze, G.N.: 1980 b, Astrofizika, 16, 687.Google Scholar
Sharpless, S.: 1954, Astrophys. J., 119, 334.CrossRefGoogle Scholar