Peremennye Zvezdy

Peremennye Zvezdy (Variable Stars) 38, No. 5, 2018

Received 4 December; accepted 19 December.

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Novae in 2018: Official Announcement of GCVS Names

E. V. Kazarovets1, N. N. Samus1,2

  1. Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya Str. 48, 119017 Moscow, Russia; e-mail: helene@inasan.ru, samus@sai.msu.ru

  2. Sternberg Astronomical Institute of Lomonosov Moscow University, University Ave. 13, 119234 Moscow, Russia


GCVS names are announced for 14 galactic Novae discovered in 2018.

According to an agreement between the team of the General Catalogue of Variable Stars (GCVS; Samus et al. 2017) and the Central Bureau of Astronomical Telegrams (CBAT) reached in 1998, GCVS names for galactic Novae and some other variable stars of special interest can be given, upon BAT suggestion, between regular Name-lists of Variable Stars. These GCVS names are supposed to be announced in IAU Circulars or Central Bureau Electronic Telegrams and then enter the next regular Name-list. This practice meets approval of the astronomical community, new names begin to be frequently used by researchers immediately after the variable's discovery.

Kazarovets and Samus (2017) announced GCVS names for 20 Novae discovered in 2015-2017. As reported in Kazarovets and Samus (2017), recent Novae, currently often initially announced not in the CBAT sources, frequently remained not noticed by the CBAT at all.

The present paper announced official GCVS names for 14 Novae. For the Novae discovered in 2018, the GCVS names have not been announced in the IAU Circulars. Necessary information on the new discoveries is presented in Table 1. These stars will enter the GCVS Name-list No. 82, now already submitted.

Acknowledgments: Our GCVS work is supported, in part, by the Programme P28 of the Presidium of Russian Academy of Sciences. We have made use of information resources provided by the ASAS-SN survey (Shappee et al. 2014; Kochanek et al. 2017). We would like to specially thank Hitoshi Yamada, Patrick Schmeer, and other astronomers who turned our attention to discoveries of Novae not announced in the IAU Circulars.

Table 1. New GCVS names for Novae

GCVS name
Nova Coordinates (J2000.0) Type Range, mag   JD of maximum Ref.
    h, m, s          

V0435 CMa
N CMa 2018 07 13 45.84 -21 12 31.3 NA 2458202 1
V0906 Car N Car 2018 10 36 15.41 -59 35 53.6 NA 2458199 2
FM Cir N Cir 2018 13 53 27.57 -67 25 01.0 NA 2458139 3
V0408 Lup N Lup 2018 15 38 43.80 -47 44 41.0 NA 2458273 4
V0357 Mus N Mus 2018 11 26 15.00 -65 31 24.2 NA 2458134 5
V0556 Nor PNV J16143400-5330050 16 14 32.91 -53 30 15.0 NA 2458407 6
V3664 Oph PNV J17244011-2421463 17 24 39.96 -24 21 47.4 N: 2458163 7
V3665 Oph N Oph 2018 No. 2 17 14 02.61 -28 49 23.7 NA 2458190 8
V3666 Oph N Oph 2018 No. 3 17 42 24.01 -20 53 08.9 NA 2458344 9
V5857 Sgr N Sgr 2018 18 04 09.45 -18 03 55.8 NA 2458218 10
V1661 Sco N Sco 2018 17 18 06.37 -32 04 27.7 NA 2458137 11
V1662 Sco N Sco 2018 No. 2 16 48 49.62 -44 57 03.2 NA 2458159 12
V1663 Sco ASASSN-18ds 17 03 47.51 -38 16 57.1 NA 2458181 13
V0613 Sct N Sct 2018 18 29 22.94 -14 30 44.2 NA 2458300 14


References in Table 1: 1. Soma et al. (2018). 2. Stanek et al. (2018b). 3. Seach et al. (2018). 4. Kaufman et al. (2018b). 5. Kaufman et al. (2018a). 6. Kaufman et al. (2018c). 7. Aydi et al. (2018). 8. Nakano et al. (2018c). 9. Jacques et al. (2018). 10. Nakano et al. (2018a). 11. Nakano et al. (2018d). 12. Nakano et al. (2018b). 13. Stanek et al. (2018a). 14. Nakano et al. (2018e).

References:

Aydi, E., Buckley, D.A.H., Mohamed, S., Whitelock, P.A., 2018, Astronomer's Telegram, No. 11338

Jacques, C., Barros, J., Pimentel, E., et al., 2018, CBET, No. 4540

Kaufman, R., Guido, E., Norschese, A., et al., 2018a, CBET, No. 4472

Kaufman, R., Kiyota, S., Pearce, A., et al., 2018b, CBET, No. 4520

Kaufman, R., Kiyota, S., Pearce, A., et al., 2018c, CBET, No. 4568

Kazarovets, E.V., Samus, N.N., 2017, Peremennye Zvezdy/Variable Stars, 37, No. 4

Kochanek, C.S., Shappee, B.J., Stanek, K.Z., et al., 2017, Publ. Astron. Soc. Pacific, 129, 104502

Nakano, S., Kojima, T., Nishimura, H., et al., 2018a, CBET, No. 4507

Nakano, S., Nishimura, H., Kiyota, S., et al., 2018b, CBET, No. 4488

Nakano, S., Nishimura, H., Kojima, T., et al., 2018c, CBET, No. 4492

Nakano, S., Nishimura, H., Noguchi, T., et al., 2018d, CBET, No. 4481

Nakano, S., Sakurai, Y., Kiyota, S., et al., 2018e, CBET, No. 4530

Samus, N.N., Kazarovets, E.V., Durlevich, O.V., Kireeva, N.N., Pastukhova, E.N., 2017, Astronomy Reports, 61, 80

Seach, J., Pearce, A., Chapman, A., et al., 2018, CBET, No. 4482

Shappee, B.J., Prieto, J.L., Grupe, D., et al., 2014, Astrophys. J., 788, No. 1, article id. 48

Soma, M., Nakamura, Yu., Schmeer, P., et al. 2018, CBET, No. 4499

Stanek, K.Z., Kochanek, C.S., Shields, J.V., et al., 2018a, Astronomer's Telegram, No. 11348

Stanek, K.Z., Luckas, P., Waagen, E.O., et al., 2018b, CBET, No. 4498





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