Modeling of the SiO Circumstellar Maser: Rate Coefficients for the Vibrationally‐Rotationally Inelastic Scattering of H+SiO-Reference-Cited by-同舟云学术

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Modeling of the SiO Circumstellar Maser: Rate Coefficients for the Vibrationally‐Rotationally Inelastic Scattering of H+SiO

Published:2006-03 Issue:1 Volume:639 Page:204-209
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Palov A. P.,Gray M. D.,Field D.,Balint‐Kurti G. G.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference30 articles.

1. Collisional rates for vibrational-rotational transitions in circumstellar SiO masers

2. Erratum - Collisional Rates for Vibrational / Rotational Transitions in Circumstellar SIO Masers

3. Dynamical modeling of long-period variable star atmospheres

4. Sudden rotation calculations of atom–molecule scattering

5. Accuracy of the IOS approximation for highly inelastic RT collisional energy transfer. CO-Ar

Cited by 6 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. Magnetic Field Structure of Orion Source I;The Astrophysical Journal;2020-06-24

2. Ro-vibrational analysis of SiO in UV-irradiated environments;Molecular Astrophysics;2018-11

3. Resolving the extended atmosphere and the inner wind of Mira (oCeti) with long ALMA baselines;Astronomy & Astrophysics;2016-05-27

4. Electron collision with the silicon monoxide (SiO) molecule using theR-matrix method;Journal of Physics B: Atomic, Molecular and Optical Physics;2009-04-21

5. SiO maser emission in Miras;Monthly Notices of the Royal Astronomical Society;2009-03-21

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