Methanol masers in environments of three massive protostars

dc.creatorBartkiewicz, A.
dc.creatorSzymczak, M.
dc.creatorvan Langevelde, H. J.
dc.date2004-11-30
dc.date.accessioned2026-07-07T02:16:06Z
dc.date.available2026-07-07T02:16:06Z
dc.descriptionWe present the first EVN maps of 6.7 GHz methanol masers of three high-mass protostar candidates selected from the Torun unbiased survey of the Galactic plane. A variety of linear and arc like structures was detected. A number of maser clusters with projected sizes of 20-100 AU show monotonic velocity gradients. Some of them are roughly perpendicular to the major axes of these structures and can arise behind shock fronts.
dc.description4 pages, 3 figures. Proceedings of the 7th European VLBI Network Symposium held in Toledo, Spain on October 12-15, 2004. Editors: R. Bachiller, F. Colomer, J.-F. Desmurs, P. de Vicente (Observatorio Astronomico Nacional), p. 187-190. Needs evn2004.cls
dc.identifierhttps://arxiv.org/abs/astro-ph/0412002
dc.identifierhttp://arxiv.org/abs/astro-ph/0412002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8658
dc.subjectAstrophysics
dc.titleMethanol masers in environments of three massive protostars
dc.typetext

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