Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2211
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dc.contributor.authorPandian, J.D.-
dc.contributor.authorGoldsmith, P.F.-
dc.contributor.authorDeshpande, A.A.-
dc.date.accessioned2007-03-16T09:59:47Z-
dc.date.available2007-03-16T09:59:47Z-
dc.date.issued2007-02-10-
dc.identifier.citationAstrophysical Journal, 2007, Vol.656, p 255-274en
dc.identifier.issn1538-4357 (online)-
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2289/2211-
dc.descriptionRestricted Access. Articles older than 2 years are open to all at the journal site (alternative location)en
dc.description.abstractWe present the results of an unbiased survey for 6.7 GHz methanol masers in the Galactic plane carried out using the 305 m Arecibo radio telescope. A total of 18.2 deg2 was surveyed with uniform sampling at 35.2deg<=l<=53.7deg, |b|<=0.41deg. The large collecting area of Arecibo and the sensitive C-Band High receiver allowed the survey to be complete at the level of 0.27 Jy, making this the most sensitive blind survey carried out to date. We detected a total of 86 sources, 48 of which are new detections. Most of the new detections have a peak flux density below 2 Jy. Many methanol masers are clustered, reflecting the formation of massive stars in clusters.en
dc.format.extent996681 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe University of Chicago Press for the American Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2007ApJ...656..255Pen
dc.relation.urihttp://arxiv.org/abs/astro-ph/0702147en
dc.relation.urihttp://dx.doi.org/10.1086/510512en
dc.rights2007 American Astronomical Societyen
dc.subjectMasersen
dc.subjectRadio Lines: ISMen
dc.subjectStars: Formationen
dc.subjectSurveysen
dc.titleThe Arecibo Methanol Maser Galactic Plane Survey. I. Dataen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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