1. Электронный научный архив УрФУ
  2. 00. Общеуниверситетские коллекции
  3. Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC
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dc.contributor.authorTsvetkov, D. Y.en
dc.contributor.authorBalanutsa, P. V.en
dc.contributor.authorLipunov, V. M.en
dc.contributor.authorVolkov, I. M.en
dc.contributor.authorTuchin, O. A.en
dc.contributor.authorKudelina, I. P.en
dc.contributor.authorPruzhinskaya, M. V.en
dc.contributor.authorGorbovskoy, E. S.en
dc.contributor.authorKornilov, V. G.en
dc.contributor.authorBelinskii, A. A.en
dc.contributor.authorTyurina, N. V.en
dc.contributor.authorYurkov, V. V.en
dc.contributor.authorSergienko, Y. P.en
dc.contributor.authorTlatov, A. G.en
dc.contributor.authorParkhomenko, A. V.en
dc.contributor.authorDormidontov, D. V.en
dc.contributor.authorSenik, V. A.en
dc.contributor.authorKrushinskii, V. V.en
dc.date.accessioned2022-05-12T08:19:44Z-
dc.date.available2022-05-12T08:19:44Z-
dc.date.issued2011-
dc.identifier.citationPhotometric Observations of the Supernova 2009nr / D. Y. Tsvetkov, P. V. Balanutsa, V. M. Lipunov et al. — DOI 10.1134/S0081543820020017 // Astronomy Letters. — 2011. — Vol. 37. — Iss. 11. — P. 775-782.en
dc.identifier.issn1063-7737-
dc.identifier.otherAll Open Access, Green3
dc.identifier.urihttp://elar.urfu.ru/handle/10995/111617-
dc.description.abstractWe present the results of our UBVRI CCD photometry for the second brightest supernova of 2009, SN 2009nr, discovered during a sky survey with the telescopes of the MASTER robotic network. Its light and color curves and bolometric light curves have been constructed. The light-curve parameters and the maximum luminosity have been determined. SN 2009nr is shown to be similar in light-curve shape and maximum luminosity to SN 1991T, which is the prototype of the class of supernovae Ia with an enhanced luminosity. SN 2009nr exploded far from the center of the spiral galaxy UGC 8255 and most likely belongs to its old halo population. We hypothesize that this explosion is a consequence of the merger of white dwarfs. © 2011 Pleiades Publishing, Ltd.en
dc.description.sponsorshipThis work was supported by the Ministry of Science of the Russian Federation (State contract no. 02.740.11.0249), the “Dynasty” Foundation of noncommercial programs, and the Russian Foundation for Basic Research (project no. 10-02-00249a). IRAF is distributed by the NOAO, which are operated by the AURA, Inc., under contract with the NSF.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherPleiades Publishing Ltden
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceAstron. Lett.2
dc.sourceAstronomy Lettersen
dc.subjectSUPERNOVAEen
dc.subjectSUPERNOVA REMNANTSen
dc.titlePhotometric Observations of the Supernova 2009nren
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/submittedVersionen
dc.identifier.doi10.1134/S0081543820020017-
dc.identifier.scopus80155150246-
local.contributor.employeeTsvetkov, D.Y., Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russian Federation; Balanutsa, P.V., Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russian Federation; Lipunov, V.M., Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russian Federation; Volkov, I.M., Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russian Federation; Tuchin, O.A., Children's Additional Education Center of Industrial District, ul. Novo-Vokzal'naya 203a, Samara, Russian Federation; Kudelina, I.P., Blagoveshchensk State Pedagogical University, ul. Lenina 104, Blagoveshchensk 675000, Russian Federation; Pruzhinskaya, M.V., Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russian Federation; Gorbovskoy, E.S., Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russian Federation; Kornilov, V.G., Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russian Federation; Belinskii, A.A., Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russian Federation; Tyurina, N.V., Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russian Federation; Yurkov, V.V., Blagoveshchensk State Pedagogical University, ul. Lenina 104, Blagoveshchensk 675000, Russian Federation; Sergienko, Y.P., Blagoveshchensk State Pedagogical University, ul. Lenina 104, Blagoveshchensk 675000, Russian Federation; Tlatov, A.G., Kislovodsk Solar Station, Main Astronomical Observatory, Russian Academy of Sciences, Kislovodsk 357700, Russian Federation; Parkhomenko, A.V., Kislovodsk Solar Station, Main Astronomical Observatory, Russian Academy of Sciences, Kislovodsk 357700, Russian Federation; Dormidontov, D.V., Kislovodsk Solar Station, Main Astronomical Observatory, Russian Academy of Sciences, Kislovodsk 357700, Russian Federation; Senik, V.A., Kislovodsk Solar Station, Main Astronomical Observatory, Russian Academy of Sciences, Kislovodsk 357700, Russian Federation; Krushinskii, V.V., Ural State University, ul. Mira 19, Yekaterinburg, Russian Federationen
local.description.firstpage775-
local.description.lastpage782-
local.issue11-
local.volume37-
local.contributor.departmentSternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russian Federation; Children's Additional Education Center of Industrial District, ul. Novo-Vokzal'naya 203a, Samara, Russian Federation; Blagoveshchensk State Pedagogical University, ul. Lenina 104, Blagoveshchensk 675000, Russian Federation; Kislovodsk Solar Station, Main Astronomical Observatory, Russian Academy of Sciences, Kislovodsk 357700, Russian Federation; Ural State University, ul. Mira 19, Yekaterinburg, Russian Federationen
local.identifier.pure9242924-
local.identifier.eid2-s2.0-80155150246-
local.fund.rffi10-02-00249-
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