A tentative identification of methanol as the progenitor of the 3.52-μm emission feature in several comets-Reference-Cited by-同舟云学术

A tentative identification of methanol as the progenitor of the 3.52-μm emission feature in several comets

Published:1991-09 Issue:1 Volume:93 Page:122-134
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Hoban Susan,Mumma Michael,Reuter Dennis C.,DiSanti Michael,Joyce R.R.,Storrs Alex

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference28 articles.

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

2. Observations of parent molecules in Comets P/Brorsen-Metcalf (1989o), Austin (1989c1) and Levy (1990c) at millimeter wavelengths: HCN, H2S, H2CO and CH3OH;Bockelée-Morvan;ESA SP-315,1990

3. Observations of Recent Comets;Bockelée-Morvan,1990

4. Spectroscopy of emission features near 3 μm in Comet Wilson (1986l);Brooke;Astrophys. J.,1989

5. Detection of the 3.4 μm emission feature in Comets P/Brorsen-Metcalf and Okazaki-Levy-Rudenko (1989r) and an observational summary;Brooke;Astron. J.,1991

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