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Characteristics of the interstellar medium as deduced from low frequency recombination line observations

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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.format.extent537937 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationAstronomy and Astrophysics, 1975, Vol.43, p465-468.en
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/2289/1592
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

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