Water formation in early solar nebula: I. Quasi-stationary cloud core-Reference-Cited by-同舟云学术

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Water formation in early solar nebula: I. Quasi-stationary cloud core

Published:2014-08 Issue: Volume:98 Page:216-232
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Tornow C.,Gast P.,Pelivan I.,Kupper S.,Kührt E.,Motschmann U.

Funder

Helmholtz Alliance on Planetary Evolution and Life

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference110 articles.

1. Protoatmospheres and surface environment of protoplanets;Abe;Earth Moon Planets,2011

2. The birth environment of the solar system;Adams;Annu. Rev. Astron. Astrophys.,2010

3. Evolution of molecular abundance in gaseous disks around young stars: depletion of CO Molecules;Aikawa;Astrophys. J.,1996

4. Evolution of molecular abundances in protoplanetary disks;Aikawa;Astrophys. J.,1997

5. Molecular evolution and star formation: from prestellar cores to protostellar cores;Aikawa;Astrophys. J.,2008

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The Composition of the Protosolar Disk and the Formation Conditions for Comets;Comets as Tracers of Solar System Formation and Evolution;2017

2. Structural and physical properties of condensed H2O systems up to 2 GPa: A brief review;Moscow University Physics Bulletin;2016-01

3. The Composition of the Protosolar Disk and the Formation Conditions for Comets;Space Science Reviews;2015-06-26

4. Simulating the D/H ratio of water formed in the early solar nebula;GEOCHEMICAL JOURNAL;2014

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