Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1361
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dc.contributor.authorOmar, A.-
dc.contributor.authorDwarakanath, K.S.-
dc.contributor.authorAnantharamaiah, K.R.-
dc.date.accessioned2006-06-12T11:08:47Z-
dc.date.available2006-06-12T11:08:47Z-
dc.date.issued2002-
dc.identifier.citationBulletin of the Astronomical Society of India, 2002, Vol.30, p749-750en
dc.identifier.issn0340-9523-
dc.identifier.urihttp://hdl.handle.net/2289/1361-
dc.descriptionPresented at the 21st meeting of the Astronomical Society of India, Pune, 2002.en
dc.description.abstractThis project aims to image a subset of galaxies in the nearby group Eridanus in HI emission and in radio continuum using the GMRT. The typical resolution of HI images will be $\sim$1 kpc with a 3$\sigma$ sensitivity to HI mass of a few times 10$^{7}$ M$_\odot$. The rotation curves obtained using the HI velocity field together with the 2MASS magnitudes in the near infrared will be used to construct the Tully-Fisher relation for this group. High resolution (sub-kpc) multi-frequency radio continuum images will be used to study star-formation rates, radio morphologies and spectral indices of Eridanus galaxies. About half of the galaxies have already been observed and further observations on some late type galaxies are proposed with the GMRT. We present here the HI image and the rotation curve for a member of this group viz. NGC 1385.en
dc.format.extent396949 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe Astronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2002BASI...30..749Oen
dc.rights(2002) by the Astronomical Society of India.en
dc.subjectGalaxy - H Ien
dc.subjectGalaxy - ISMen
dc.subjectgroup - galaxyen
dc.titleA GMRT H I imaging survey of the ERIDANUS group of galaxiesen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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