Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-12-17
Astronomy and Astrophysics
Astrophysics
11 pages, 7 figures, to appear in PASJ
Scientific paper
We photometrically observed the 2003 June superoutburst of GO Gom. The mean superhump period was 0.063059(13) d. The resultant data revealed that (1) the obtained light curve contained a precursor, (2) a plateau stage of the object lasted 8 days, which is remarkably shorter than that of ordinary SU UMa-type dwarf novae, and (3) the amplitude of the superoutburst was less than 5 mag, which is unpredictably small when taking into account the fact that the supercycle of GO Com is about 2800 days. In order to explain these anomalies, a mass elimination process from the accretion disk, such as evaporation, may play an important role.
Cook Lewis M.
Imada Akira
Ishioka Ryoko
Jones Christopher P.
Kato Taichi
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