RRI Banner

The Arecibo methanol maser galactic plane survey

dc.contributor.authorPandian, J D
dc.contributor.authorGoldsmith, P F
dc.contributor.authorDeshpande, A A
dc.date.accessioned2009-07-01T10:34:19Z
dc.date.available2009-07-01T10:34:19Z
dc.date.issued2007
dc.descriptionRestricted Access.en
dc.description.abstractThe Arecibo Methanol Maser Galactic Plane Survey (AMGPS) is a blind survey for 6.7 GHz methanol masers in a section of the Galactic plane visible from the Arecibo radio telescope. The survey for these signposts of massive star formation is complete at a flux density level of 0.27 Jy making it the most sensitive blind survey for methanol masers carried out to date, and resulted in the detection of 86 methanol masers, 48 of which are new discoveries. The properties of methanol masers discovered in the survey are consistent with their being associated with early phases of massive star formation. The data also show the tangent point of the Carina-Sagittarius spiral arm to be around a Galactic longitude of 49.6°.en
dc.identifier.citationProceedings of the IAU symposium 242: Astrophysical masers and their environments. Eds. J M Chapman & W A Baan. p208en
dc.identifier.urihttp://hdl.handle.net/2289/3785
dc.language.isoenen
dc.publisherCambridge University Pressen
dc.relation.urihttp://adsabs.harvard.edu/abs/2007IAUS..242..208Pen
dc.relation.urihttp://dx.doi.org/10.1017/S1743921307012987en
dc.rights2007 International Astronomical Unionen
dc.subjectsurveysen
dc.subjectGalaxy: structureen
dc.subjectstars: formationen
dc.titleThe Arecibo methanol maser galactic plane surveyen
dc.typeArticleen

Files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
2007_IAUSymposium_242_p208.pdf
Size:
129.59 KB
Format:
Adobe Portable Document Format
Description:
Open Access