History of the solar-type protostar IRAS 16293–2422 as told by the cyanopolyynes-Reference-Cited by-同舟云学术

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History of the solar-type protostar IRAS 16293–2422 as told by the cyanopolyynes

Published:2016-12-20 Issue: Volume:597 Page:A40
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Jaber Al-Edhari A.,Ceccarelli C.,Kahane C.,Viti S.,Balucani N.,Caux E.,Faure A.,Lefloch B.,Lique F.,Mendoza E.,Quenard D.,Wiesenfeld L.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201629506/pdf

Reference59 articles.

1. CS, HC3N, and CH3CCH multi-line analyses toward starburst galaxies

2. The Chemical Composition of the Sun

3. Shock Chemistry in the Young Bipolar Outflow L1157

4. Detection of HC[TINF]11[/TINF]N in the Cold Dust Cloud TMC-1

5. Hyperfine excitation of HCN by H2 at low temperature

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4. Cyanopolyyne Chemistry in the L1544 Prestellar Core: New Insights from GBT Observations;The Astrophysical Journal;2023-02-01

5. Reactions O(³P, ¹D) + HCCCN(X¹Σ⁺) (Cyanoacetylene): Crossed-Beam and Theoretical Studies and Implications for the Chemistry of Extraterrestrial Environments;The Journal of Physical Chemistry A;2023-01-13

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