Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1356
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dc.contributor.authorSridharan, T.K.-
dc.date.accessioned2006-06-12T10:20:22Z-
dc.date.available2006-06-12T10:20:22Z-
dc.date.issued1993-09-
dc.identifier.citationBulletin of the Astronomical Society of India, 1993, Vol.21, p339-345en
dc.identifier.issn0304-9523-
dc.identifier.urihttp://hdl.handle.net/2289/1356-
dc.description.abstractThe 10.4m millimeter-wave telescope of the Raman Research Institute (RRI) has been in operation since 1988. It can observe over the 3-mm atmospheric transmission window (80-115 GHz) where rotational transitions of many molecules including CO lie. Dual polarization cryogenic receivers developed at RRI are in use with the telescope. Filter bands and acousto-optic spectrometers are employed as back-ends for carrying out molecular spectroscopy. Study of SiO masers in late type stars, CO line observations of molecular clouds near massive stars, in the Gould's belt and near supernova remnants and millimeter wave recombination lines are some of the research programs undertaken. Future plans include the development of a four beam receiver to speed up mapping observations.en
dc.format.extent636948 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe Astronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1993BASI...21..339Sen
dc.rights(1993) by the Astronomical Society of India. Scanned images provided by the NASA ADS Data System.en
dc.subjectInterstellar masersen
dc.subjectMolecular cloudsen
dc.subjectRadio astronomyen
dc.subjectRadio equipmentsen
dc.subjectRadio sources (Astronomy)en
dc.subjectRadio telescopesen
dc.subjectCircuit diagramsen
dc.subjectMillimeter wavesen
dc.subjectMolecular spectroscopyen
dc.subjectParabolic antennasen
dc.titleThe RRI 10.4m millimeter-wave telescopeen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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