X-Ray and Infrared Emissions from Accreting Magnetic White Dwarfs : A Model for AM Herculis

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概要

• 論文の詳細を見る

• We have constructed the detailed numerical models of AM Her. The models assume that the material transferred from a binary companion forms a shock heated accretion column on the magnetic pole of a white dwarf. The structure of the accretion column and the energy spectrum emitted are calculated numerically. White dwarfs with moderately low surface magnetic field, <2×10^7G, are most likely to reproduce the observed features of the spectrum.

• 理論物理学刊行会の論文
• 1980-12-25

著者

• SHIMIZU Akira

  Department of Electrical and Electronic Engineering, Tokyo Institute of Technology

• KATO Mariko

  Department of Astronomy, Keio University

• Kato Mitsuhiro

  Kanagawa Fish. Res. Institute

• HOSHI Reiun

  Department of Physics, Rikkyo University

• Hoshi Reiun

  Department Of Physics Kyoto University

• WADA Toshi-aki

  Department of Physics, Rikkyo University

• SUZUKI Masatoki

  Department of Physics, Rikkyo University

• Wada Toshiaki

  Department Of Applied Physics Tokyo University Of Agriculture And Technology:(present Address) Depar

• Wada Toshi-aki

  Department Of Physics Rikkyo University

• Suzuki Masatoki

  Department Of Physics Rikkyo University

• Shimizu Akira

  Department Of Dermatology Gunma University Graduate School Of Medicine

• HO-SHI Reiun

  Department of Physics, Rikkyo University

• Shimizu Akira

  Department Of Biological Sciences Graduate School Of Science And Engineering Tokyo Metropolitan Univ

• Shimizu Akira

  Department Of Basic Science The University Of Tokyo

• Shimizu Akira

  Deparment Of Physics Rikkyo University

• SHIMIZU Akira

  Department of Physics, Rikkyo University

• Kato Mitsuhiro

  Department of Mathematical Sciences, Osaka Prefecture University

• Wada Takahiro

  General Information Processing Center

• Wada Toshiaki

  Department of Applied Chemistry, College of Engineering, University of Osaka Prefecture

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