The results of UBVR observations of some Is variable stars - T Tauri-type objects and AE/BE Herbig stars

Details The results of UBVR observations of some Is variable stars - T Tauri-type objects and AE/BE Herbig stars The results of UBVR observations of some Is variable stars - T Tauri-type objects and AE/BE Herbig stars

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..951k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Sept.-Oct. 1988, p. 951-970. In Russian.

Physics

9

Herbig-Haro Objects, Stellar Physics, Stellar Spectrophotometry, T Tauri Stars, Ubv Spectra, Variable Stars, A Stars, B Stars, Electrophotometry

Scientific paper

The photometric features of Is variable stars are compared on the basis of UBVR data. The InT stars studied formed three distinct groups. The first group was made up of the well-known YY Ori-type stars RW Aur, S CrA, DL Tau, and GQ Lup. The second group was composed of GM Aur, UY Aur, BP Tau, DF Tau, and DO Tau. The third group included DI Cep, RY Tau, CX Tau, DI Tau, and DN Tau.

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