Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Australia National University, Australia
Department of Mathematics, The Australian National University, Canberra, ACT 0200, Australia
Department of Mathematics, Australian National University, Canberra, ACT 0200, Australia
Mount Stromlo and Siding Spring Observatoires, Canberra, Australia
The Australian National University Astrophysical Theory Centre, School of Mathematical Sciences, Canberra, ACT 0200, Australia
Leicester, University, England
Department of Mathematics, Australian National University, Canberra ACT 0200, Australia.
Department of Mathematics, The Australian National University, Canberra, Australia
Mathematical Sciences Institute, The Australian National University, Canberra, Australia
Department of Mathematics, Australian National University, ACT 0200, Canberra, Australia
Astrophysical Theory Centre, School of Mathematical Sciences, The Australian National University, Canberra, ACT 0200, Australia
Mathematical Sciences Institute, The Australian National University, ACT 0200, Australia
Department of Mathematics, School of Mathematical Sciences, The Australian National University, ACT 0200, Australia of Mathematics and Astrophysical Theory Centre, Australian National University, Canberra, ACT 0200, Australia
Australian National Univ., Canberra, Australia
Department of Mathematics, Mathematical Sciences Institute, The Australian National University, ACT 0200, Australia
The Astrophysical Theory Centre, School of Mathematical Sciences, The Australian National University, Canberra, ACT 0200, Australia
Australian National Univ., Canberra.
Australian National Univ., Canberra, Australia; Leicester Univ., United Kingdom
Department of Applied Mathematics, Australian National University, Canberra, ACT 0200, Australia & Astrophysics Programme & Department of Mathematics, Sc
1H 1752+08: the lowest field AM Herculis system?
1RXS J0823.6-2525: a new ultramassive magnetic white dwarf
A 56 MG field at the second pole in VV Puppis
A centered dipole model for the high field magnetic white dwarf GRW + 70 deg 8247
A Model for the Optical Continuum and Balmer Emission Lines in Intermediate Polars
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Profile ID: LFWR-SCP-P-168701