X-BAND VLA-ASTERISK OBSERVATIONS OF COMET HYAKUTAKE (C 1996 B2) AND IMPLICATIONS FOR NUCLEAR PROPERTIES/

Citation
Yr. Fernandez et al., X-BAND VLA-ASTERISK OBSERVATIONS OF COMET HYAKUTAKE (C 1996 B2) AND IMPLICATIONS FOR NUCLEAR PROPERTIES/, Planetary and space science, 45(6), 1997, pp. 735-739
Citations number
20
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00320633
Volume
45
Issue
6
Year of publication
1997
Pages
735 - 739
Database
ISI
SICI code
0032-0633(1997)45:6<735:XVOOCH>2.0.ZU;2-L
Abstract
The results of our observations during the close approach of comet C/1 996 B2 (Hyakutake) using Very Large Array (VLA) at a wavelength of 3.5 5 cm (X-band) are presented. The scientific goals were to; observe the thermal microwave continuum from the nucleus and constrain the comet' s nuclear properties. The 12 h track allows 3-sigma upper limits to be placed on the emission that are about a factor of four lower than any previous VLA observation of a comet's continuum. With the caveat that some assumptions about the microwave emissivity, the temperature, and the thermal conductivity must be made, the effective radius of Hyakut ake's nucleus is constrained to be less than 3.0 km, which provides an addition to the sparse body of knowledge on long-period cometary nucl ei. Since the observations overlap several of the ROSAT observations o f this comet, the strength of the microwave flux is estimated from the X-ray emitting region of the to place constraints on possible emissio n mechanisms. (C) 1997 Elsevier Science Ltd.