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[vsnet-campaign 391] TT Ind further brightens
TT Ind further brightens
Further brightening has been observed, reaching the brightest level in
the past. The object is at mag 18 in quiescence, so the present outburst
has a chance of a superoutburst (or a large-amplitude SS Cyg star).
Time-resolved photometry is strongly needed to clarify its nature.
Follow-up information will be presented in vsnet-campaign-dn.
YYYYMMDD(UT) mag observer
20000722.467 <146 (P. Williams)
20000722.635 <144 (R. Stubbings)
20000723.419 138 (R. Stubbings)
20000723.477 143 (P. Williams)
20000724.531 132 (A. Pearce)
20000724.541 127 (R. Stubbings)
20000724.819 128 (A. Pearce)
Regards,
Taichi Kato
VSNET Collaboration team
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp