1. RRI Digital Repository
  2. 04. Astronomy and Astrophysics
  3. Research Papers (A&A)
Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1409
Full metadata record
DC FieldValueLanguage
dc.contributor.authorAnantharamaiah, K.R.-
dc.contributor.authorErickson, W.C.-
dc.contributor.authorPayne, H.E.-
dc.contributor.authorKantharia, N.G.-
dc.date.accessioned2006-07-07T06:16:21Z-
dc.date.available2006-07-07T06:16:21Z-
dc.date.issued1994-08-
dc.identifier.citationAstrophysical Journal, 1994, Vol.430, p682-689en
dc.identifier.issn0004-637X-
dc.identifier.issn1538-4357 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/1409-
dc.description.abstractWe present observations of the C270 alpha carbon recombination line, 21 cm neutral hydrogen line and (12)CO (J = 1 right arrow 0) molecular line toward Cas A. A comparison of the distribution of recombination line optical depths over the face of Cas A with that of H I optical depths and molecular line emission favors the association of C270 alpha regions with H I rather than molecular clouds. The association makes it possible to self-consistently determine several physical parameters of the clouds by combining the recombination line and 21 cm H I measurements.en
dc.format.extent1337670 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?1994ApJ...430..682Aen
dc.rights(1994) by the American Astronomical Society. Scanned images provided by the NASA ADS Data System.en
dc.subjectABUNDANCEen
dc.subjectCASSIOPEIA Aen
dc.subjectH I REGIONSen
dc.subjectHYDROGENen
dc.subjectINTERSTELLAR MATTERen
dc.subjectRADIO EMISSIONen
dc.subjectRYDBERG SERIESen
dc.subjectASTRONOMICAL MODELSen
dc.subjectCOSMOLOGYen
dc.subjectNEUTRAL GASESen
dc.subjectRECOMBINATION REACTIONSen
dc.subjectSPECTRUM ANALYSISen
dc.subjectVERY LARGE ARRAY (VLA)en
dc.titleHigh Rydberg state carbon recombination lines toward Cassiopeia A: 332 MHz VLA observations and comparison with H I and molecular linesen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
1994 ApJ V430 p682-689.pdf8p.1.31 MBAdobe PDFView/Open
Show simple item record


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.