Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

CBAT "Transient Object Followup Reports"

TCP J19500635-0736530

TCP J19500635-0736530   2020 06 17.5852*  19 50 06.35 -07 36 53.0   5.7 U             Aql       I 0



2020 06 17.58

This is the Mira variable GY Aquilae, which is currently bright, according to recent ASAS-SN Sky Patrol (Shappee et al. 2014ApJ...788...48S and Kochanek et al. 2017PASP..129j4502K) data at https://asas-sn.osu.edu/light_curves/3cd664d7-6dce-4265-b1ba-39daa8a6ddd8 – another light curve at https://asas-sn.osu.edu/variables/d292fc7e-0d5c-5be7-971e-4ea0d0f03a07 —— Patrick Schmeer (Saarbrücken-Bischmisheim, Germany)




2020 06 17.586

Sorry,Thank you for pointing out:K.Itagaki



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