Carbon Atom Condensation on NH<sub>3</sub>–H<sub>2</sub>O Ices. An Alternative Pathway to Interstellar Methanimine and Methylamine-Reference-Cited by-同舟云学术

Carbon Atom Condensation on NH₃–H₂O Ices. An Alternative Pathway to Interstellar Methanimine and Methylamine

Published:2024-05-06 Issue:19 Volume:128 Page:3874-3889
ISSN:1089-5639
Container-title:The Journal of Physical Chemistry A
language:en
Short-container-title:J. Phys. Chem. A

Author:

Molpeceres Germán¹²^ORCID,Tsuge Masashi³^ORCID,Furuya Kenji¹⁴,Watanabe Naoki³^ORCID,San Andrés David⁵^ORCID,Rivilla Víctor M.⁵,Colzi Laura⁵^ORCID,Aikawa Yuri¹

Affiliation:

1. Department of Astronomy, Graduate School of Science, The University of Tokyo, Tokyo 113 0033, Japan

2. Departamento de Astrofísica Molecular, Instituto de Física Fundamental (IFF-CSIC), C/Serrano 121, 28006 Madrid, Spain

3. Institute of Low Temperature Science, Hokkaido University, Sapporo, Hokkaido 060-0819, Japan

4. National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan

5. Centro de Astrobiología (CAB), INTA-CSIC, Carretera de Ajalvir km 4, Torrejón de Ardoz, 28850 Madrid, Spain

Funder

Ministerio de Econom??a y Competitividad

Comunidad de Madrid

European Commission

Deutsche Forschungsgemeinschaft

Ministry of Education, Culture, Sports, Science and Technology

Publisher

American Chemical Society (ACS)

Link

https://pubs.acs.org/doi/pdf/10.1021/acs.jpca.3c08286

Reference92 articles.

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3. Hydrogenation reactions in interstellar CO ice analogues

4. A THREE-PHASE CHEMICAL MODEL OF HOT CORES: THE FORMATION OF GLYCINE

5. Formation of Complex Organic Molecules in Hot Molecular Cores through Nondiffusive Grain-surface and Ice-mantle Chemistry

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