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Long-term evolution of the outgassing of comet Hale-Bopp from radio observations
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
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1997 (English)In: EARTH MOON AND PLANETS, ISSN 0167-9295, Vol. 78, no 1-3, 5-11 p.Article in journal (Refereed) Published
Abstract [en]

C/1995 O1 (Hale-Bopp) has been observed on a regular basis since August 1995 at millimetre and submillimetre wavelengths using IRAM, JCMT, CSO and SEST radio telescopes. The production rates of eight molecular species (CO, HCN, CH3OH, H2CO, H2S, CS, CH3CN

Place, publisher, year, edition, pages
KLUWER ACADEMIC PUBL , 1997. Vol. 78, no 1-3, 5-11 p.
Keyword [en]
comets; C/1995 O1 (Hale-Bopp); radio observations; molecules; CARBON-MONOXIDE; FORMALDEHYDE; RATES
Identifiers
URN: urn:nbn:se:uu:diva-36626OAI: oai:DiVA.org:uu-36626DiVA: diva2:64525
Note
Addresses: Biver N, Univ Hawaii, IfA, Honolulu, HI 96822 USA. Observ Paris Meudon, Meudon, France. Joint Astron Ctr, Hilo, HI 96720 USA. Inst Radio Astron Millimetr, Granada, Spain. Inst Radio Astron Millimetr, Grenoble, France. Observ Bordeaux, Bordeaux,Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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