Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1578
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dc.contributor.authorEllingsen, S.P.-
dc.contributor.authorVon Bibra, M.L.-
dc.contributor.authorMcCulloch, P.M.-
dc.contributor.authorNorris, R.P.-
dc.contributor.authorDeshpande, A.A.-
dc.contributor.authorPhillips, C.J.-
dc.date.accessioned2006-12-14T07:17:53Z-
dc.date.available2006-12-14T07:17:53Z-
dc.date.issued1996-05-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 1996, Vol.280, p378-396en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2289/1578-
dc.descriptionSorry, the full text of this article is not available here. Please click on the alternative location to access it.en
dc.description.abstractWe report the results of the first complete survey of an area of the Galactic plane for maser emission from the 6.7-GHz 5_1--〉6_0 A^+ transition of CH_3OH. The survey covers a 10.6-deg^2 region of the Galactic plane in the longitude range 325 deg-335 deg and latitude range -0.˚53-0.˚53. The survey is sensitive to masers with a peak flux density greater than ~2.6 Jy. The weakest maser detected has a peak flux density of 2.3 Jy, and the strongest a peak flux density of 425 Jy. We detected a total of 50 distinct masers, 26 of which are new detections. We show that many 6.7-GHz CH_3OH masers are not associated with IRAS sources, and that some are associated with sources that have colours differing from those of a typical ultracompact HII (UCHII) region. We estimate that the number of UCHII regions in the Galaxy is significantly more than suggested by IRAS-based estimates, possibly by more than a factor of 2.en
dc.format.extent8338 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherBlackwell Publishing for the Royal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1996MNRAS.280..378Een
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996MNRAS.280..378E&link_type=ARTICLE&db_key=ASTen
dc.rights(1996) Royal Astronomical Societyen
dc.subjectMASERS,en
dc.subjectSURVEYS,en
dc.subjectSTARS: FORMATION,en
dc.subjectHII REGIONS,en
dc.subjectISM: MOLECULES,en
dc.subjectRADIO LINES: ISMen
dc.titleA survey of the galactic plane for 6.7-GHz methanol masers - I. l=325 deg-335 deg b=-0.˚53-0.˚53en
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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