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Long-term evolution of the outgassing of comet Hale-Bopp from radio observations

Biver, N (author)
Uppsala universitet,Institutionen för astronomi och rymdfysik
Bockelee-Morvan, D (author)
Colom, P (author)
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Crovisier, J (author)
Germain, B (author)
Lellouch, E (author)
Davies, JK (author)
Dent, WRF (author)
Moreno, R (author)
Paubert, G (author)
Wink, J (author)
Despois, D (author)
Lis, DC (author)
Mehringer, D (author)
Benford, D (author)
Gardner, M (author)
Phillips, TG (author)
Gunnarsson, M (author)
Rickman, H (author)
Winnberg, A (author)
Bergman, P (author)
Johansson, LEB (author)
Ra, (author)
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 (creator_code:org_t)
KLUWER ACADEMIC PUBL, 1997
1997
English.
In: EARTH MOON AND PLANETS. - : KLUWER ACADEMIC PUBL. - 0167-9295. ; 78:1-3, s. 5-11
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • 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

Keyword

comets; C/1995 O1 (Hale-Bopp); radio observations; molecules; CARBON-MONOXIDE; FORMALDEHYDE; RATES

Publication and Content Type

ref (subject category)
art (subject category)

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