Developing a self-consistent AGB wind model – I. Chemical, thermal, and dynamical coupling-Reference-Cited by-同舟云学术

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Developing a self-consistent AGB wind model – I. Chemical, thermal, and dynamical coupling

Published:2018-09-20 Issue:4 Volume:482 Page:5052-5077
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Boulangier Jels¹^ORCID,Clementel N¹,van Marle A J²,Decin L¹,de Koter A¹³

Affiliation:

1. Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium

2. Department of Physics, School of Natural Sciences UNIST, Ulsan 44919, Korea

3. Anton Pannenkoek Institute for Astronomy, Universiteit van Amsterdam, Science Park 904, NL-1098 XH Amsterdam, the Netherlands

Funder

European Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/482/4/5052/26909173/sty2560.pdf

Reference98 articles.

1. Modeling primordial gas in numerical cosmology

2. A periodic shock wave model for Mira variable atmospheres

3. The physical state of primordial intergalactic clouds

4. Collision-induced absorption coefficients of H2pairs at temperatures from 60 K to 1000 K

5. High-temperature (1000–7000 K) collision-induced absorption of H2 pairs computed from the first principles, with application to cool and dense stellar atmospheres

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