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- W43596523 abstract "We present time resolved V-band CCD photometry of the dwarf nova V485 Cen. It is found that the optical brightness during quiescence is modulated with a period of 59 m . Brightness variations with the same period may also by present during outburst. The observed spectrum in quiescence is fairly typical for a dwarf nova. However, we find that the He I line at 5876 A is much stronger relative to Hα than is the case in other cataclysmic variables. We discuss the nature of the 59 m period in terms of (i) the rotation period of the white dwarf; (ii) the orbital period of the system" @default.
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- W43596523 date "1993-01-01" @default.
- W43596523 modified "2023-09-26" @default.
- W43596523 title "A 59m photometric period in the dwarf nova V 485 Centauri" @default.
- W43596523 hasPublicationYear "1993" @default.
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