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http://hdl.handle.net/2289/4118
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DC Field | Value | Language |
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dc.contributor.author | Deguchi, Shuji | - |
dc.contributor.author | Koike, Kazutaka | - |
dc.contributor.author | Balasubramanyam, R. | - |
dc.date.accessioned | 2011-08-23T09:38:57Z | - |
dc.date.available | 2011-08-23T09:38:57Z | - |
dc.date.issued | 2009-09 | - |
dc.identifier.citation | ASP Conference Series, 2009, Vol.407, p260 | en |
dc.identifier.uri | http://hdl.handle.net/2289/4118 | - |
dc.description | Restricted 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.260 | en |
dc.description.abstract | Meterwave 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.iso | en | en |
dc.publisher | Astronomical Society of the Pacific | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/2009ASPC..407..260D | en |
dc.rights | 2009 Astronomical Society of the Pacific | en |
dc.title | Nature of meterwave luminous objects and search for electron-cyclotron maser emission | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2009_ASPCS_407_260.pdf Restricted Access | Restricted access | 155.52 kB | Adobe PDF | View/Open Request a copy |
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