[vsnet-alert 28167] TCPJ15030519+2202041: early superhump and rapid decay
TCPJ15030519+2202041: shows early superhump and rapid decay now Itoh-san, Moriyama-san, Hiraga-san, Funada-san, Magnus Larsson, and Josch Hambsch have newly reported their observations. According to the data, this object showed an early superhump with an amplitude of 0.03. Furthermore, this object has a superhump period of 0.03041(1). Now, this object shows rapid fading since May 15. AM CVn-type dwarf novae show the second outburst after an interval of several to more than ten days. This is a perfect opportunity to observe the growing superhump, so it is very important to observe this object even if it gets faint. best regard, Hiromasa Hoke
TCPJ15030519+2202041: is still in quiescent interval before the second superoutburst Itoh-san, Moriyama-san, Hiraga-san, Funada-san, Magnus Larsson, and Josch Hambsch have newly reported their observations. According to the data, this object is still in quiescent interval before the second superoutburst. The current magnitude is 19~20. AM CVn-type dwarf novae show the second outburst after an interval of several to more than ten days. Continued observations are encouraged to catch the onset of the second superoutburst. best regard, Hiromasa Hoke On 2026/05/16 18:43, Hiromasa Hoke via vsnet-alert wrote:
TCPJ15030519+2202041: shows early superhump and rapid decay now
Itoh-san, Moriyama-san, Hiraga-san, Funada-san, Magnus Larsson, and Josch Hambsch have newly reported their observations. According to the data, this object showed an early superhump with an amplitude of 0.03. Furthermore, this object has a superhump period of 0.03041(1). Now, this object shows rapid fading since May 15. AM CVn-type dwarf novae show the second outburst after an interval of several to more than ten days. This is a perfect opportunity to observe the growing superhump, so it is very important to observe this object even if it gets faint.
best regard, Hiromasa Hoke
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Hiromasa Hoke