OUTBURST CYCLICITY OF DWARF NOVA VZ AQUARII
New linear elements for outbursts of VZ Aqr from 1904 to 1987 were obtained with P0 = 50.4053d. Two states of outburst activity are distinguished with cycle lengths 47.128d and 55.041d, replacing each other during Π = 13.2yr and accompanied by a maximum brightness changes. Instability parameters of...
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| Format: | Article |
| Language: | English |
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Odessa I. I. Mechnykov National University
2017-07-01
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| Series: | Odessa Astronomical Publications |
| Online Access: | http://oap.onu.edu.ua/article/view/105786 |
| Summary: | New linear elements for outbursts of VZ Aqr from 1904 to 1987 were obtained with P0 = 50.4053d. Two states of outburst activity are distinguished with cycle lengths 47.128d and 55.041d, replacing each other during Π = 13.2yr and accompanied by a maximum brightness changes. Instability parameters of VZ Aqr – lg P, lg P/Po, lg Π and lg N0 agree well with a dependence of these parameters on lg P0 derived by the author for other dwarf Novae. |
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| ISSN: | 1810-4215 |