July 2023 - vsnet-campaign-nova - ooruri.kusastro.kyoto-u.ac.jp

[vsnet-campaign-nova 2299] VY Scl fading
by Taichi Kato 26 Jul '23

26 Jul '23

VY Scl fading As pointed out by Rod Stubbings. YYYYMMDD(UT) mag observer 20230614.4047 13.381g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230616.2739 13.649g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230617.3584 13.664g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230619.2794 13.115g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230623.0134 13.247g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230624.0234 13.387g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230625.2558 13.569g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230626.2966 13.750g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230629.2510 13.650g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230630.4389 14.046g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230702.2937 13.475g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230703.3364 13.478g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230705.2270 13.728g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230708.4395 13.474g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014)) 20230711.5528 141 (Rod Stubbings) 20230712.5667 140 (Rod Stubbings) 20230715.6410 144 (Rod Stubbings) 20230716.7431 141 (Rod Stubbings) 20230717.5549 144 (Rod Stubbings) 20230725.505 <153 (Rod Stubbings)

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[vsnet-campaign-nova 2298] No 0.1-d period in V2491 Cyg
by Taichi Kato 13 Jul '23

13 Jul '23

No 0.1-d period in V2491 Cyg https://ui.adsabs.harvard.edu/abs/2011A%26A...530A..70D/abstract "On the progenitor system of Nova V2491 Cygni" No such period was detected in the ZTF data. Two time-resolved runs in the ZTF data did not show any sign of such a period. The detection by this paper was probably spurious. There was no sign of the reported possible spin period (see Zemko et al. 2015).

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[vsnet-campaign-nova 2297] NSV21190: eclipsing symbiotic star currently undergoing symbiotic nova outburst?
by Taichi Kato 07 Jul '23

07 Jul '23

NSV21190: eclipsing symbiotic star currently undergoing symbiotic nova outburst? Yamamoto had reported brightening of this object in April. YYYYMMDD(UT) mag observer 20230422.744 132c (Minoru Yamamoto) Tadashi Kojima-san has reported that the object has been bright for months. object YYYYMMDD(UT) mag code NSV21190 20230331.758 128c Tko.VSOLJ NSV21190 20230517.629 128c Tko.VSOLJ NSV21190 20230617.503 128c Tko.VSOLJ NSV21190 20230706.553 127c Tko.VSOLJ This object has been suggested to be a large-amplitude variable star TerzV910 (suspected to be a Mira star based on IRAS identification). ASAS-SN data https://asas-sn.osu.edu/sky-patrol/coordinate/d5a29922-5bc0-4e1e-824e-086ac… and ATLAS observations suggest that this object appears to be an eclipsing symbiotic object, rather than a Mira star, which became active (at least) in in 2017. The minima occurred JD 2458240:, 2458660, 2459060: (P about 410 d?). The object once became faint in later 2020-later 2021, and then brightened to the current bright state. A shallow minimum around JD 2459830 during the present bright state may be an eclipse (the period then is around 400 d). The object was faint during ASAS-3 observations (2000-2009). The object is currently slowly brightening and would be another symbiotic nova (the shallow eclipse may be explained by a nova photosphere). The position is somewhat different between 2MASS and Gaia: 2MASS 171453.440 -283746.69 (2000.0) 15.129 12.170 9.707 171453.437 -283746.95 (2000.0) Gaia_DR2_4107611274955676672 plx=-(-) dismod=- pmra=-(-) pmdec=-(-) G=19.526 BP=20.104 RP=17.634 171453.437 -283746.96 (2000.0) Gaia_EDR3_4107611274955676672 plx=2.187(0.418) dismod=8.3 pmra=-6.604(0.411) pmdec=-7.609(0.337) G=19.598 BP=20.516 RP=18.301 I used the 2MASS location.

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