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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3797
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dc.contributor.authorKameswara Rao, N-
dc.contributor.authorVenugopal, V. R-
dc.contributor.authorPatnaik, A. R-
dc.date.accessioned2008-09-22T16:59:06Z-
dc.date.available2008-09-22T16:59:06Z-
dc.date.issued1987-09-
dc.identifier.citationJournal of Astrophysics and Astronomy , Vol. 8, No. 3, pp. 227 - 230en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3797-
dc.description.abstractVLA observations at 6 cm have been obtained for three hydrogen-deficient objects (Upsilon Sgr, V 348 Sgr, and Abell 58). Abell 58 was also observed at 2 cm. Only upper limits to the flux density could be set for these sources. A new radio source at 6 cm was found in the field of Upsilon Sgr. The upper limit for 6-cm flux density of V 348 Sgr sets an upper limit to its reddening as E(B-V) = 0.65 or less. The hydrogen-deficient planetary nebula A 58 shows much lower radio flux than expected from the IR radio flux-density relationship of planetary nebulae.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1987JApA....8..227Ken
dc.subjectHydrogenen
dc.subjectRadio astronomyen
dc.subjectStellar compositionen
dc.subjectStellar spectrophotometryen
dc.subjectVery large array (vla)en
dc.subjectCentimeter wavesen
dc.subjectInfrared radiationen
dc.subjectPlanetary nebulaeen
dc.subjectRadiant flux densityen
dc.titleFurther VLA observations of hydrogen deficient starsen
dc.typeArticleen
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