1. Электронный научный архив УрФУ
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dc.contributor.authorBayandina, O. S.en
dc.contributor.authorBurns, R. A.en
dc.contributor.authorKurtz, S. E.en
dc.contributor.authorShakhvorostova, N. N.en
dc.contributor.authorVal'Tts, I. E.en
dc.date.accessioned2021-08-31T14:58:50Z-
dc.date.available2021-08-31T14:58:50Z-
dc.date.issued2019-
dc.identifier.citationVLA Overview of the Bursting H2O Maser Source G25.65+1.05 / O. S. Bayandina, R. A. Burns, S. E. Kurtz, et al. — DOI 10.3847/1538-4357/ab3fa4 // Astrophysical Journal. — 2019. — Vol. 884. — Iss. 2. — 140.en
dc.identifier.issn0004637X-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access, Green3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85075188893&doi=10.3847%2f1538-4357%2fab3fa4&partnerID=40&md5=04289a9ac834c9376b411bbb6b158f4e
dc.identifier.otherhttp://arxiv.org/pdf/1812.11353m
dc.identifier.urihttp://elar.urfu.ru/handle/10995/101669-
dc.description.abstractThe source G25.65+1.05 (RAFGL7009S, IRAS 18316-0602) is the least studied of the three regions of massive star formation known to show exceptionally powerful H2O maser bursts. We report spectral line observations of the H2O maser at 22 GHz, the methanol maser transitions at 6.7, 12.2, and 44 GHz, and the continuum in these same frequency bands with The Karl G. Jansky Very Large Array at the post-burst epoch of 2017. For the first time, maps of 22 GHz H2O and 44 GHz CH3OH maser spots are obtained and the absolute position of the 22 GHz H2O bursting feature is determined with milliarcsecond precision. We detected four continuum components, three of which are closely spaced in a linear orientation, suggesting a physical link between them. © 2019. The American Astronomical Society. All rights reserved..en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherInstitute of Physics Publishingen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceAstrophys. J.2
dc.sourceAstrophysical Journalen
dc.subjectEVOLUTIONen
dc.subjectMASERSen
dc.titleVLA Overview of the Bursting H2O Maser Source G25.65+1.05en
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.3847/1538-4357/ab3fa4-
dc.identifier.scopus85075188893-
local.contributor.employeeBayandina, O.S., Joint Institute for VLBI ERIC, Oude Hoogeveensedijk 4, PD Dwingeloo, 7991, Netherlands, Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Leninskiy Prospekt 53, Moscow, 119333, Russian Federation
local.contributor.employeeBurns, R.A., Joint Institute for VLBI ERIC, Oude Hoogeveensedijk 4, PD Dwingeloo, 7991, Netherlands, Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan, Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu Daejeon, 34055, South Korea
local.contributor.employeeKurtz, S.E., Instituto de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Apartado Postal 3-72, Morelia, 58089, Mexico
local.contributor.employeeShakhvorostova, N.N., Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Leninskiy Prospekt 53, Moscow, 119333, Russian Federation, Astronomical Observatory, Institute for Natural Sciences and Mathematics, Ural Federal University, Kuybyshev st. 48, Ekaterinburg, 620026, Russian Federation
local.contributor.employeeVal'Tts, I.E., Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Leninskiy Prospekt 53, Moscow, 119333, Russian Federation
local.issue2-
local.volume884-
dc.identifier.wos000501779300020-
local.contributor.departmentJoint Institute for VLBI ERIC, Oude Hoogeveensedijk 4, PD Dwingeloo, 7991, Netherlands
local.contributor.departmentAstro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Leninskiy Prospekt 53, Moscow, 119333, Russian Federation
local.contributor.departmentMizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan
local.contributor.departmentKorea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu Daejeon, 34055, South Korea
local.contributor.departmentInstituto de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Apartado Postal 3-72, Morelia, 58089, Mexico
local.contributor.departmentAstronomical Observatory, Institute for Natural Sciences and Mathematics, Ural Federal University, Kuybyshev st. 48, Ekaterinburg, 620026, Russian Federation
local.identifier.purebbfcc6fc-c8a9-4610-8059-c6f93d3028a9uuid
local.identifier.pure11347409-
local.description.order140-
local.identifier.eid2-s2.0-85075188893-
local.identifier.wosWOS:000501779300020-
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