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BIMA array observations of comet Hyakutake: upper limit to the 2.7 mm continuum emission

Identifieur interne : 000825 ( Main/Curation ); précédent : 000824; suivant : 000826

BIMA array observations of comet Hyakutake: upper limit to the 2.7 mm continuum emission

Auteurs : Imke De Pater [États-Unis] ; Lewis E. Snyder [États-Unis] ; David M. Mehringer [États-Unis] ; Melvyn Wright [États-Unis] ; Jeffrey M. Veal [États-Unis] ; Yanga R. Fernández [États-Unis] ; Patrick Palmer [États-Unis] ; Michael F. A'Hearn [États-Unis]

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RBID : ISTEX:505FDD97548ACB1904BF2D94888A0B243267B2F1

Abstract

Comet Hyakutake (C/1996 B2) was observed with the BIMA array at a wavelength of 2.7 mm. An upper limit of 6.3 mJy per beam is reported, which, if all due to thermal emission from the nucleus of the comet itself, translates into an upper limit of 2.5 km for the comet's radius. The results are compared with detections at sub-mm wavelengths (Jewitt and Matthews, Astron. J. 113, 1145–1151, 1997), and the likelihood of detecting comet Hale-Bopp at mm-cm wavelengths is commented on.

Url:
DOI: 10.1016/S0032-0633(97)00078-0

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ISTEX:505FDD97548ACB1904BF2D94888A0B243267B2F1

Le document en format XML

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<div type="abstract" xml:lang="en">Comet Hyakutake (C/1996 B2) was observed with the BIMA array at a wavelength of 2.7 mm. An upper limit of 6.3 mJy per beam is reported, which, if all due to thermal emission from the nucleus of the comet itself, translates into an upper limit of 2.5 km for the comet's radius. The results are compared with detections at sub-mm wavelengths (Jewitt and Matthews, Astron. J. 113, 1145–1151, 1997), and the likelihood of detecting comet Hale-Bopp at mm-cm wavelengths is commented on.</div>
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