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Master: 3 OTстатья
- Авторы: Balanutsa P., Lipunov V., Buckley D., Tlatov A., Gorbovskoy E., Tyurina N., Kuuznetsov A., Kornilov V., Kuvshinov D., Popova E., Vlasenko D., Shumkov V., Potter S., Kniazev A., Budnev N., Gress O., Ivanov K., Senik V., Dormidontov D., Parhomenko A.V.
- Журнал: The Astronomer’s Telegram
- Том: 9322
- Год издания: 2016
- Аннотация: MASTER: 3 OT ATel #9322; P. Balanutsa, V. Lipunov (Lomonosov MSU), D. Buckley (SAAO), A. Tlatov (KSS, Pulkovo Observatory), E. Gorbovskoy, N. Tyurina, A. Kuznetsov, V. Kornilov, D. Kuvshinov, E. Popova, D. Vlasenko, V. Shumkov (Lomonosov Moscow State University, SAI), S. Potter, A. Kniazev (South African Astronomical Observatory), N. Budnev, O. Gress, K. Ivanov (API, Irkutsk State University), V. Senik, D. Dormidontov, A. V. Parhomenko (Kislovodsk Solar Station of the Pulkovo Observatory) on 5 Aug 2016; 01:41 UT Credential Certification: Nataly Tyurina (tiurina@sai.msu.ru) Subjects: Optical, Request for Observations, Cataclysmic Variable, Transient, Variables MASTER OT J213350.58+065122.5 discovery - possibly dwarf nova outburst, ampl>4.2, no source in VIZIER MASTER-Kislovodsk auto-detection system ( Lipunov et al., "MASTER Global Robotic Net", Advances in Astronomy, 2010, 30L ) discovered OT source at (RA, Dec) = 21h 33m 50.58s +06d 51m 22.5s on 2016-07-27.94690 UT. The OT unfiltered magnitude is 17.8m (limit 18.0m). The OT is seen in 4 images. We reobserved it at MASTER-SAAO on 2016-08-02 23:15:48 with m_OT=18.1 We have reference image without OT on 2014-11-20.70189 UT with unfiltered magnitude limit 20.6m. Spectral observations are required. The discovery and reference images are available at: http://observ.pereplet.ru/images/MASTEROTJ213350.58+065122.5.jpg MASTER OT J211343.51-644019.4 discovery - OT with Ampl>3.4m MASTER-SAAO auto-detection system discovered OT source at (RA, Dec) = 21h 13m 43.51s -64d 40m 19.4s on 2016-08-01.93853 UT. The OT unfiltered magnitude is 18.6m (limit 20.2m). The OT is seen in 7 images. We have reference image without OT on 2015-10-06.86088 UT with unfiltered magnitude limit 20.2m. There is only GSC2.3.2 star with blue j=20.35 during its previous outburst. Taking into account 22m upper limit from POSS images, current outburst is with ampl>3.4m Spectral observations are required. The discovery and reference images are available at: http://master.sai.msu.ru/static/OT/211343.51-644019.4.png MASTER OT J151925.64-183101.5 discovery - dwarf nova outburst, Ampl>2.6m MASTER-SAAO auto-detection system discovered OT source at (RA, Dec) = 15h 19m 25.64s -18d 31m 01.5s on 2016-08-01.81626 UT. The OT unfiltered magnitude is 19.4m (limit 20.4m). The OT is seen in 3 images. There is no minor planet at this place. We have reference image without OT on 2016-07-03.90478 UT with unfiltered magnitude limit 20.6m. There is GSC2.3.2 star with blue j=20.34 and red f=19.8 during last outburst (22m POSS limit between them), so current outburst is more then 2.6m. Spectral observations are required. The discovery and reference images are available at: http://master.sai.msu.ru/static/OT/151925.64-183101.5.png
- Добавил в систему: Липунов Владимир Михайлович