Radiation driven-dust hydrodynamics in late-phase AGB stars-Reference-Cited by-同舟云学术

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Radiation driven-dust hydrodynamics in late-phase AGB stars

Published:2023-10 Issue: Volume:45 Page:100766
ISSN:2213-1337
Container-title:Astronomy and Computing
language:en
Short-container-title:Astronomy and Computing

Author:

Zargarnezhad H.,Myers R.J.,Speck A.K.,McFarland J.A.^ORCID

Funder

University of Missouri

National Science Foundation

Publisher

Elsevier BV

Subject

Computer Science Applications,Astronomy and Astrophysics,Space and Planetary Science

Reference63 articles.

1. Astrophysics. Nuclear Transformations, Stellar Interiors, and Nebulae;Aller,1954

2. Dust formation in winds of long-period variables - V. The influence of micro-physical dust properties in carbon stars;Andersen;Astron. Astrophys.,2003

3. The multiphase particle-in-cell (MP-PIC) method for dense particulate flows;Andrews;IJMF,1996

4. The mass loss of C-rich giants ******;Bergeat;Astron. Astrophys.,2005

5. Fundamentals of Heat and Mass Transfer, Vol. 997;Bergman,2011

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