The 2.5–12 μm spectrum of comet halley from the IKS-VEGA experiment-Reference-Cited by-同舟云学术

The 2.5–12 μm spectrum of comet halley from the IKS-VEGA experiment

Published:1988-12 Issue:3 Volume:76 Page:404-436
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Combes M.,Moroz V.I.,Crovisier J.,Encrenaz T.,Bibring J.-P.,Grigoriev A.V.,Sanko N.F.,Coron N.,Crifo J.F.,Gispert R.,Bockelée-Morvan D.,Nikolsky Yu.V.,Krasnopolsky V.A.,Owen T.,Emerich C.,Lamarre J.M.,Rocard F.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference94 articles.

1. Discovery of organic grains in comet Wilson;Allen;Nature,1987

2. Nuclear and electron dynamics in the photodissociation of water;Andresen;J. Chem. Phys.,1984

3. The comet Halley flyby IR sounder “IKS”;Arduini;Adv. Space Res.,1982

4. The abundance of sulphur in coments;Azoulay,1986

5. Spectroscopy of the 3.4 micron emission feature in comet Halley;Baas;Astrophys. J.,1986

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