Upper limits on the pulsed radio emission from the Geminga pulsar at 35 & 327 MHz

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1543

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DC Field	Value	Language
dc.contributor.author	Ramachandran, R.	-
dc.contributor.author	Deshpande, A.A.	-
dc.contributor.author	Indrani, C.	-
dc.date.accessioned	2006-11-27T06:01:23Z	-
dc.date.available	2006-11-27T06:01:23Z	-
dc.date.issued	1998-11	-
dc.identifier.citation	Astronomy and Astrophysics, 1998, Vol.339, p787-790	en
dc.identifier.issn	0004-6361	-
dc.identifier.uri	http://hdl.handle.net/2289/1543	-
dc.description.abstract	We report here our observations at 35 MHz and 327 MHz made in the direction of the 〉~mma-Ray pulsar Geminga. Based on the observed absence of any significant pulsed emission from this source above our detection thresholds at the two frequencies, we obtain useful upper-limits for the average flux to be 75-100 mJy at 35 MHz, and 0.2-0.3 mJy at 327 MHz. We discuss a few possible reasons for the ``radio-quiet'' nature of this pulsar at frequencies other than around 100 MHz.	en
dc.format.extent	95560 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Springer-Verlag	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998A%26A...339..787R&link_type=ARTICLE&db_key=AST	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/9808234	en
dc.rights	(1998) by European Southern Observatory	en
dc.subject	PULSARS: INDIVIDUAL: J0633+1746	en
dc.title	Upper limits on the pulsed radio emission from the Geminga pulsar at 35 & 327 MHz	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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