On the dust boundary at Halley and volatility of cometary organics

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 500, 2002, Pages 579-582

  Oberc, P ^a  

^a Borowiec Astrogeodynamic Observatory   (Poland)

Author keywords

[No Author keywords available]

Indexed keywords

AGGREGATES; DISINTEGRATION; DUST; HEAT CONDUCTION; SOLAR SYSTEM; SUBLIMATION;

DUST BOUNDARY;

ASTROPHYSICS;

EID: 0036664987     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

References (8)

1. -10 g) in comet P/Halley's coma. Astron. Astrophys. Vol. 187, 753-760.
2. Obere, P. 1996. Disintegration of dust aggregates as origin of the boundaries in Halley's coma: Derivation of the sublimation parameters. Icarus, Vol. 124, 195-208.
3. Weidenschilling, S. J. 1997. The origin of comets in the solar nebula: a unified model. Icarus Vol. 127, 290-306.
4. Huebner, W. F. 1970. Dust from cometary nuclei. Astron. Astrophys. Vol. 5, 286-297.
5. Crifo, J. F. 1991. Hydrodynamic models of the collisional coma. In Comets in the post-Halley era. (R. L. Newburn, M. Neugebauer, and J. Rahe, Eds.), Vol. 2, pp. 937-989. Kluwer Acad. Publishers.
6. Grün, E., and E. K. Jessberger 1990. Dust. In Physics and Chemistry of Comets. (W. E. Huebner, Ed.), pp. 113-176. Springer-Verlag.
7. Krueger, F. R., A. Korth, and J. Kissel 1991. The organic matter of comet Halley as inferred by joint gas and solid phase analyses. Space Sci. Rev. Vol. 56, 167-175.
8. Kissel, J., F. R. Krueger, and K. Roessler 1997. Organic chemistry in comets from remote and in-situ observations. In Comets and the origin and evolution of life. (P. J. Thomas, C. F. Chyba, and C. P. McKay, Eds.), pp. 69-109. Springer-Verlag.