SUPEROUTBURST OF V1504 CYGNI IN 2003
The photometry of the SU UMa-type dwarf nova V1504 Cygni during the superoutburst is performed. The star displayed the superoutburst decay at a rate about 0.15 mag / day. Evolution of super-humps during the superoutbursts is discussed.
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| Format: | Article |
| Language: | English |
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Odessa I. I. Mechnykov National University
2017-03-01
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| Series: | Odessa Astronomical Publications |
| Online Access: | http://oap.onu.edu.ua/article/view/96930 |