The Low State of Z CMa

UNCG Author/Contributor (non-UNCG co-authors, if there are any, appear on document)
Anatoly S. Miroshnichenko, Associate Professor (Creator)
Institution
The University of North Carolina at Greensboro (UNCG )
Web Site: http://library.uncg.edu/

Abstract: Z CMa, a remarkable star, has been attracting the attention of observers for many years. Its photometric behaviour summarized at least twice recently (Covino et al., 1984. Kolotilov, 1991) often shows new details. After the period of a relative stability in early 80-es (Kilkenny et al., 1985, Herbst et al., 1987) two visual brightness increases of the star was observed. The first one occurred in 1985 (Shevchenko, 1989), and the second was in 1986-1987 (Miroshnichenko and Yudin, 1992).

Additional Information

Publication
Commissions 27 and 42 of the IAU Information Bulletin on Variable Stars 3937
Language: English
Date: 1993
Keywords
stars, Z CMa, photometric behavior