Isotopic ethyl cyanide $^{\mathsf{13}}$CH$_\mathsf{3}$CH$_\mathsf{2}$CN, CH$_\mathsf{3}$$^{\mathsf{13}}$CH$_\mathsf{2}$CN, and CH$_\mathsf{3}$CH$_\mathsf{2}$$^{\mathsf{13}}$CN: laboratory rotational spectrum and detection in Orion-Reference-Cited by-同舟云学术

Isotopic ethyl cyanide $^{\mathsf{13}}$CH$_\mathsf{3}$CH$_\mathsf{2}$CN, CH$_\mathsf{3}$$^{\mathsf{13}}$CH$_\mathsf{2}$CN, and CH$_\mathsf{3}$CH$_\mathsf{2}$$^{\mathsf{13}}$CN: laboratory rotational spectrum and detection in Orion

Published:2007-02-27 Issue:1 Volume:466 Page:255-259
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Demyk K.,Mäder H.,Tercero B.,Cernicharo J.,Demaison J.,Margulès L.,Wegner M.,Keipert S.,Sheng M.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20066955/pdf

Reference30 articles.

1. Molecular abundances in OMC-1 - The chemical composition of interstellar molecular clouds and the influence of massive star formation

2. A λ = 1.3 Millimeter Aperture Synthesis Molecular Line Survey of Orion Kleinmann-Low

3. Cernicharo, J. 1985, Internal IRAM report (Granada: IRAM)

4. A Molecular Line Survey of Orion KL in the 350 Micron Band

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