Protoalgols and quasi-algols

Details Protoalgols and quasi-algols Protoalgols and quasi-algols

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993astl...19..125s&link_type=abstract

Astronomy Letters, Vol. 19, p. 125-130; Pis'ma v Astronomicheskij Zhurnal (ISSN 0320-0108), vol. 19, no. 4, p. 334-347. In Russ

Astronomy and Astrophysics

Astronomy

6

Binary Stars, Molecular Clouds, Stellar Composition, Stellar Evolution, T Tauri Stars, Accretion Disks, Infrared Astronomy

Scientific paper

Observational characteristics of 11 extremely young close binary systems associated with accretion disks are given. Some of these stars have been known as irregular variables of the T Tauri or Ae/Be Herbig type (V 628 Cas, BO Cep, IL Cep, TY CrA, T Ori, RZ Psc, and VY Tau). Others (BM Ori, EY Ori, and V 1016 Ori) are associated with the extremely young Orion cluster; two of them are components of the Orion Trapezium complex (Theta-prime Ori). The nonstationary accretion from the disk to the components of these stars can partially account for the observed phenomena.

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