Photometry of the long period dwarf nova GY Hya
نویسندگان
چکیده
منابع مشابه
Outburst Photometry of the Eclipsing Dwarf Nova GY Cancri
We observed the ROSAT-selected eclipsing dwarf nova GY Cnc (=RX J0909.8+1849) during the 2001 November outburst. We refined the orbital period to be 0.17544251(5) d. The fading portion of the outburst was indistinguishable from those of typical dwarf novae with similar orbital periods. However, the signature of orbital humps (or a hot spot) was far less prominently observed in the orbital light...
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ژورنال
عنوان ژورنال: New Astronomy
سال: 2017
ISSN: 1384-1076
DOI: 10.1016/j.newast.2017.03.001