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C/1995 O1 (Hale-Bopp): Gas production curves and their interpretation
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
1997 (English)In: EARTH MOON AND PLANETS, ISSN 0167-9295, Vol. 79, no 1-3, 55-77 p.Article in journal (Refereed) Published
Abstract [en]

The discovery of C/1995 O1 (Hale-Bopp) at 7 AU from the Sun provided the first opportunity to follow the activity of a bright comet over a large range of heliocentric distances r(h). Production rates of a number of parent molecules and daughter species ha

Place, publisher, year, edition, pages
KLUWER ACADEMIC PUBL , 1997. Vol. 79, no 1-3, 55-77 p.
Keyword [en]
comets; cometary activity; cometary nucleus; sublimation processes; numerical modelling; LARGE HELIOCENTRIC DISTANCE; LOW THERMAL-CONDUCTIVITY; AMORPHOUS WATER ICE; COMET P-HALLEY; CARBON-MONOXIDE; NUCLEI; EVOLUTION; MODEL; SPECTRUM; RELEASE
Identifiers
URN: urn:nbn:se:uu:diva-36628OAI: oai:DiVA.org:uu-36628DiVA: diva2:64527
Note
Addresses: Bockelee-Morvan D, Observ Meudon, 5 Pl Jules Janssen, F-92190 Meudon, France. Observ Meudon, F-92190 Meudon, France. Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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