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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4118
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dc.contributor.authorDeguchi, Shuji-
dc.contributor.authorKoike, Kazutaka-
dc.contributor.authorBalasubramanyam, R.-
dc.date.accessioned2011-08-23T09:38:57Z-
dc.date.available2011-08-23T09:38:57Z-
dc.date.issued2009-09-
dc.identifier.citationASP Conference Series, 2009, Vol.407, p260en
dc.identifier.urihttp://hdl.handle.net/2289/4118-
dc.descriptionRestricted Access. Proceedings of the conference held 8-12 Dec. 2008, at National Centre for Radio Astrophysics (NCRA), TIFR, Pune, India. Edited by D. J. Saikia, D. A. Green, Y. Gupta, and T. Venturi. San Francisco: Astronomical Society of the Pacific, p.260en
dc.description.abstractMeterwave luminous objects, which are bright at the frequency 74 MHz but very faint at 1.4 GHz in VLA surveys (VLSS and NVSS), have special characteristics: very steep spectra and a distinctive distribution in the sky. They are possibly radio relics, ultra-steep spectrum radio galaxies, and Galactic objects such as pulsars, cool dwarfs, and extrasolar planets. We present a preliminary result of our attempt to identify them with possible astronomical objects. We observed several candidates for electron-cyclotron maser emission from cool dwarfs with GMRT at 235 MHz, and located the radio source VLSS 0406.1+0251 to be within 0.5'' near the M3 dwarf LSPM 0406+0251.en
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/abs/2009ASPC..407..260Den
dc.rights2009 Astronomical Society of the Pacificen
dc.titleNature of meterwave luminous objects and search for electron-cyclotron maser emissionen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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