Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Monash University
Centre for Stellar and Planetary Astrophysics, Monash University, Australia
Centre for Stellar and Planetary Astrophysics, Monash University, Melbourne, Australia
CSPA, Monash University, Australia
Monash University, Clayton, Australia
Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, 3800, Australia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei, Taiwan 10617
Monash University, Clayton, Victoria, Australia
Toronto, University, Canada
Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, Victoria 3800, Australia
Lawrence Livermore National Laboratory, Livermore, CA
Centre for Stellar and Planetary Astrophysics, Monash University
CSPA, Monash University
Monash Univ.
Department of Mathematics and Statistics, Monash University, Clayton, Victoria 3168, Australia; Institute of Astronomy, The Observatoires, Madingley Road, Cambridge CB3 0HA
Lawrence Livermore National Laboratory, Livermore; California, University, Berkeley
Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, Clayton, VIC 3800, Australia.
Department of Mathematics and Statistics, Monash University, Clayton, Victoria 3168, Australia
Centre for Stellar and Planetary Astrophysics, School of Mathematics, Monash University, Clayton, Victoria 3800, Australia
Monash University, Clayton, Australia; California, University, Berkeley
Centre for Stellar and Planetary Astrophysics, Monash University, VIC 3800, Australia Livermore National Lab., CA.
Lawrence Livermore National Lab., Livermore, CA; Monash Univ., Clayton, Australia; Cambridge Univ. Inst. of Astronomy, United Kingdom
3D hydrodynamical simulations of a proton ingestion episode in a low-metallicity asymptotic giant branch star
3D Numerical Experimentation on the Core Helium Flash of low-mass Red Giants
A large C+N+O abundance spread in giant stars of the globular cluster NGC 1851
A refined particle method for astrophysical problems
A simulation of the collapse and fragmentation of cooling molecular clouds
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