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Modeling of cometary evolution by kinetic theory: Method and first results
Uppsala University.
Uppsala University.
1996 (English)In: EARTH MOON AND PLANETS, ISSN 0167-9295, Vol. 72, no 1-3, 203-210 p.Article in journal (Other scientific) Published
Abstract [en]

Physical evolution of Jupiter family (JF) comets is considered as a simultaneous process of erosion and fading. Dynamical effects are Limited to discrete changes of the perihelion distance, that result in changes of the evaporation rate. Assuming that the

Place, publisher, year, edition, pages
KLUWER ACADEMIC PUBL , 1996. Vol. 72, no 1-3, 203-210 p.
Keyword [en]
URN: urn:nbn:se:uu:diva-85379OAI: oai:DiVA.org:uu-85379DiVA: diva2:113287
Addresses: Banaszkiewicz M, SPACE RES CTR, BARTYCKA 18A, PL-00716 WARSAW, POLAND. ASTRON OBSERV, S-75120 UPPSALA, SWEDEN.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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