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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4328
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dc.contributor.authorRajamohan, R-
dc.contributor.authorBhargavi, S. G-
dc.date.accessioned2009-02-04T16:16:26Z-
dc.date.available2009-02-04T16:16:26Z-
dc.date.issued1992-12-
dc.identifier.citationIn Lunar and Planetary Inst., Asteroids, Comets, Meteors, 1991. pp. 487 - 491en
dc.identifier.urihttp://hdl.handle.net/2248/4328-
dc.description.abstractThe CCD photometry of selected asteroids was carried out to check for possible cometary activity in them. To distinguish the asteroids with possible cometary activity from those of the main belt, each object of interest was observed in two filters; one centered on the C2 emission band at 5140A (90A bandpass) and the other centered on the nearby continuum at 4845A (65A bandpass). None of the observed asteroids appear to have any C2 emission.en
dc.language.isoenen
dc.publisherLunar and Planetary Insten
dc.relation.urihttp://adsabs.harvard.edu/abs/1992acm..proc..487Ren
dc.subjectAsteroidsen
dc.subjectAstronomical Photometryen
dc.subjectBandpass Filtersen
dc.subjectCharge Coupled Devicesen
dc.subjectCometsen
dc.subjectLight Emissionen
dc.subjectNarrowbanden
dc.subjectVisible Spectrumen
dc.titleNarrow band photometry of selected asteroidsen
dc.typeArticleen
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