Peremennye Zvezdy (Variable Stars) 38, No. 5, 2018 Received 4 December; accepted 19 December.
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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.
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).
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