A Rigid-Field Hydrodynamics approach to modelling the magnetospheres of massive stars
Open Access
- 30 October 2007
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 382 (1) , 139-157
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This publication has 49 references indexed in Scilit:
- The Young Stellar Population in M17 Revealed by ChandraThe Astrophysical Journal Supplement Series, 2007
- Magnetic Fields in Massive Stars. I. Dynamo ModelsThe Astrophysical Journal, 2001
- On the Periodic X-Ray Emission from θ[TSUP]1[/TSUP] Orionis CThe Astrophysical Journal, 1997
- The magnetic fields of the helium-weak B starsThe Astrophysical Journal Supplement Series, 1983
- The magnetic field of the helium-strong starsThe Astrophysical Journal, 1979
- Particle acceleration by astrophysical shocksThe Astrophysical Journal, 1978
- The acceleration of cosmic rays in shock fronts - IIMonthly Notices of the Royal Astronomical Society, 1978
- The acceleration of cosmic rays in shock fronts - IMonthly Notices of the Royal Astronomical Society, 1978
- Radiation-driven winds in Of starsThe Astrophysical Journal, 1975
- Magnetic fields and the structure of the solar coronaSolar Physics, 1969