Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7291
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dc.contributor.authorMishra, A-
dc.contributor.authorKantharia, N. G-
dc.contributor.authorMousumi Das-
dc.date.accessioned2018-06-13T05:37:14Z-
dc.date.available2018-06-13T05:37:14Z-
dc.date.issued2018-04-
dc.identifier.citationBulletin de la Societe Royale des Sciences de Liege, Vol. 87, pp. 365-370en_US
dc.identifier.issn0037-9565-
dc.identifier.urihttp://hdl.handle.net/2248/7291-
dc.descriptionOpen Accessen_US
dc.description.abstractIn this paper, we present radio observations of the giant low surface brightness (LSB) galaxies made using the Giant Metrewave Radio Telescope (GMRT). LSB galaxies are generally large, dark matter dominated spirals that have low star formation efficiencies and large HI gas disks. Their properties suggest that they are less evolved compared to high surface brightness galaxies. We present GMRT emission maps of LSB galaxies with an optically-identified active nucleus. Using our radio data and archival near-infrared (2MASS) and near-ultraviolet (GALEX) data, we studied morphology and star formation efficiencies in these galaxies. All the galaxies show radio continuum emission mostly associated with the centre of the galaxy.en_US
dc.language.isoenen_US
dc.publisherBulletin de la Societe Royale des Sciences de Liegeen_US
dc.relation.urihttps://popups.uliege.be/0037-9565/index.php?id=7787-
dc.rights© Bulletin de la Societe Royale des Sciences de Liege-
dc.subjectAstronomyen_US
dc.subjectAstrophysicsen_US
dc.subjectRadioen_US
dc.subjectExtragalacticen_US
dc.subjectGalaxiesen_US
dc.titleGiant Low Surface Brightness Galaxiesen_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

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