Cardiff University | Prifysgol Caerdydd ORCA
Online Research @ Cardiff 
WelshClear Cookie - decide language by browser settings

FCRAO Millimeter Continuum Observations of Comet Hale-Bopp (C/1995 O1)

Senay, M., Rownd, B., Lovell, A., Dickens, J., De Vries, C., Schloerb, F. P., Mayhew, L., Yuen, L. M. and Mauskopf, Philip Daniel 1997. FCRAO Millimeter Continuum Observations of Comet Hale-Bopp (C/1995 O1). Presented at: The 29th Annual Meeting of the Division for Planetary Sciences of the American Astronomical Society ( DPS 29th Meeting), Cambridge, MA, 28 July - 1 Aug 1997. Bulletin of the American Astronomical Society , vol. 29 (3). American Astronomical Society,

Full text not available from this repository.

Abstract

The number distribution of millimeter-size dust particles in cometary comae is difficult to establish by optical/IR means alone. However, millimeter wave continuum radio observations are sensitive to these large particles that may control the total dust coma mass. The dust/gas mass ratio derived by combining dust and spectral line observations provides very important and basic information about the physical nature of comets. In late February 1997, FCRAO expanded its intensive comet Hale-Bopp (C/1995 O1) spectral line mapping campaign with a program of millimeter wave bolometry observations of Hale-Bopp's dust coma. The observations were taken with the SuZIE multielement bolometer mounted on the FCRAO 14m radio telescope. This bolometer is capable of taking data simultaneously at wavelengths of 1.1, 1.4, and 2.1mm. Initial results from late February 1997 indicate that the equivalent blackbody cross section at 1.4mm was (6.1 +/- 0.2) x 10(4) km, implying a dust mass of M = 1.7 x 10(12) kg in the coma at the time of observation, and a dust mass production rate dM/dt = 3.2 x 10(5) kg s(-1) . For log[Q(OH)] = 30.35, this gives a dust/gas mass ratio of approximately 3.5. The slope of the continuum emission spectrum corresponds to an opacity index of beta = 1.36 +/- 0.30, intermediate between the values of beta for circumstellar dust disks and the ISM. This may be interpreted as a consequence of an evolving dust particle size distribution as the dust grains expanded outwards into the coma of comet Hale-Bopp.

Item Type: Conference or Workshop Item (Paper)
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Additional Information: Abstract only printed in the Bulletin. SESSION 32 (.06) HALE-BOPP/HYAKUTAKE I (Technical Sessions)
Publisher: American Astronomical Society
ISSN: 0002-7537
Related URLs:
Last Modified: 04 Jun 2017 07:57
URI: http://orca.cf.ac.uk/id/eprint/70407

Citation Data

Cited 4 times in Google Scholar. View in Google Scholar

Actions (repository staff only)

Edit Item Edit Item