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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2914
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dc.contributor.authorMahabal, A-
dc.contributor.authorKembhavi, A-
dc.contributor.authorSingh, K. P-
dc.contributor.authorBhat, P. N-
dc.contributor.authorPrabhu, T. P-
dc.date.accessioned2008-07-29T04:36:03Z-
dc.date.available2008-07-29T04:36:03Z-
dc.date.issued1996-02-
dc.identifier.citationAstrophysical Journal, Vol. 457, No.2, pp. 598 - 603en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/2914-
dc.description.abstractWe present the broad band surface photometry of the radio galaxy 3C 270 (NGC 4261). We find a distinct dust lane in the V - R image of the galaxy and determine its oriantation and size. We use the major axis profile of the galaxy to estimate the optical depth of the dust lane, and discuss the significance of the lane to the shape of the galaxy.en
dc.format.extent2725788 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAmerican Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996ApJ...457..598Men
dc.subjectISM: dusten
dc.subjectExtinctionen
dc.subjectGalaxies: individual alphanumeric: 3C 270en
dc.subjectGalaxies: photometryen
dc.subjectRadio continuum: Galaxiesen
dc.titleA Dust Lane in the Radio Galaxy 3C 270en
dc.typeArticleen
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