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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1592
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dc.contributor.authorShaver, P.A.-
dc.date.accessioned2006-12-15T07:17:08Z-
dc.date.available2006-12-15T07:17:08Z-
dc.date.issued1975-10-
dc.identifier.citationAstronomy and Astrophysics, 1975, Vol.43, p465-468.en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2289/1592-
dc.format.extent537937 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringer-Verlagen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1975A&A....43..465Sen
dc.rights(1975) by the European Southern Observatory. Scanned images provided by the NASA ADS Data System.en
dc.subjectCOLD GASen
dc.subjectCOSMIC PLASMAen
dc.subjectINTERSTELLAR GASen
dc.subjectRADIO SPECTRAen
dc.subjectRECOMBINATION REACTIONSen
dc.subjectABSORPTION SPECTRAen
dc.subjectBRIGHTNESS TEMPERATUREen
dc.subjectGAS DENSITYen
dc.subjectIONIZATION FREQUENCIESen
dc.subjectIONIZED GASESen
dc.subjectLINE SPECTRAen
dc.titleCharacteristics of the interstellar medium as deduced from low frequency recombination line observationsen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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