Non-thermal ion desorption from an acetonitrile (CH3CN) astrophysical ice analogue studied by electron stimulated ion desorption-Reference-Cited by-同舟云学术

Non-thermal ion desorption from an acetonitrile (CH3CN) astrophysical ice analogue studied by electron stimulated ion desorption

Published:2015 Issue:41 Volume:17 Page:27473-27480
ISSN:1463-9076
Container-title:Physical Chemistry Chemical Physics
language:en
Short-container-title:Phys. Chem. Chem. Phys.

Author:

Ribeiro F. de A.¹²³⁴⁵,Almeida G. C.¹²³⁴⁶,Garcia-Basabe Y.¹²³⁴⁷,Wolff W.⁸²³⁴,Boechat-Roberty H. M.⁹²³⁴,Rocco M. L. M.¹²³⁴

Affiliation:

1. Instituto de Química

2. Universidade Federal do Rio de Janeiro

3. Rio de Janeiro

4. Brazil

5. Instituto Federal de Educação

6. Departamento de Física

7. Instituto Latino-Americano de Ciências da Vida e da Natureza

8. Instituto de Física

9. Observatorio do Valongo

Abstract

Non-thermal desorption by electron impact constitutes an important route by which neutral and ionic fragments from simple nitrile-bearing ices may be delivered back to the gas-phase of astrophysical environments, contributing to the production of more complex molecules.

Publisher

Royal Society of Chemistry (RSC)

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy

Link

http://pubs.rsc.org/en/content/articlepdf/2015/CP/C5CP05040E

Reference72 articles.

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3. Detection of the J = 1 - 0 transition of CH3CN

4. CH 3 CN Observations toward Southern Massive Star‐forming Regions

5. METHYL CYANIDE OBSERVATIONS TOWARD MASSIVE PROTOSTARS

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