Other
Scientific paper
Apr 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..341k&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, April 1991, p. 341-346. In Russian. In Russian. In Russian.
Other
1
Early Stars, Light Curve, Peculiar Stars, Stellar Spectra, Ubv Spectra, Astronomical Photometry, Brightness Temperature, Stellar Evolution, Variable Stars
Scientific paper
The results of UBV measurements of the brightness of the variable Z CMa made between 1975 and 1990, and its hydrogen spectrum in 1983 are described. A similarity is established between the star's photometric history and its spectral variations over a period of about 60 years, on the one hand, and the nature of the afterburst evolution of eruptive young FU Ori-type stars (fuors), on the other. This conclusion is in agreement with the idea of Hartman et al. (1989), namely, that Z CMa belongs to this group. The behavior of Z CMa is presented in graphs and tables.
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