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1988 Fiscal Year Final Research Report Summary

MAGNETIC FIELDS AND ACTIVITY IN SPIRAL GALAXIES

Research Project

Project/Area Number 61460009
Research Category

Grant-in-Aid for General Scientific Research (B)

Allocation TypeSingle-year Grants
Research Field Astronomy
Research InstitutionInstitute of Astronomy, Faculty of Sci., University of Tokyo

Principal Investigator

SOFUE Yoshiaki  Fac. Sci., Univ. Tokyo, Prof., 理学部, 教授 (10022667)

Co-Investigator(Kenkyū-buntansha) HAYASHI Masahiko  ibid, Res. Fel., 理学部, 助手 (10183914)
UCHIDA Yutaka  Fac. Sci., Univ. Tokyo, Prof., 理学部, 教授 (90012814)
FUJIMOTO Mitsuaki  Fac. Sci., Nagoya Univ., Prof., 理学部, 教授 (70022580)
Project Period (FY) 1986 – 1988
KeywordsGalaxies / Our Galaxy / Magnetic fields / Activity / Galactic center / 磁場 / 電波観測
Research Abstract

The structures of magnetic fields in spiral galaxies have been investigated on the basis of observations of linear polarization of galaxies. The large-scale field orientation in the majority of nearby spiral galaxies have been shown to be bisymmetric spiral. A few exceptions are M31 and IC342 that have ring or axi-symmetric field configurations.
The formation mechaniss of these field configurations were studied based on theoretical consideration of dymano mechanism. It has been suggested that the field was originated in a protogalactic stage by winding up a large-scale intergalactic magnetic field in to the galaxy. The spiral field in the disk plane is produced by the differential rotation of the galaxy and is maintained in a steady state due to the dynamo action. On the other hand, the vertical component is accumulated toward the galactic center with the accreting interstellar gas to yield a strong vertical magnetic field.
The spiral field was shown to act an important role in the formation of the spiral structure of a galaxy, in addition to the density wave mechanism. The vertical field in the galactic center was shown to be important to produce a large-scale ejection perpendicular to the disk plane, which makes a galaxy-scale jet. In fact our observations showed the presence of a galactic center jet of 10,000 light year length.

  • Research Products

    (14 results)

All Other

All Publications (14 results)

  • [Publications] 祖父江,藤本 他: Ann.Rev.Astr.Astropys.24. 459-497 (1986)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] 祖父江 他: Publ.Astr.Soc.Japan. 39. 95-107 (1987)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] 祖父江,藤本: Astrophys.J.319. L73-76 (1987)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] 祖父江 他: Proc.W.S.on Interst.Mag.Field. 30-37 (1987)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] 祖父江,藤本: Pulel. Astr.Soc.Jpn.39. 843-848 (1987)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] 祖父江 他: Astrophys.J.(1985)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] 祖父江義明: "電波でみる銀河と宇宙" 共立出版, 168 (1988)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] 祖父江義明: "コンピュータが描く宇宙" 恒星社厚生閣, 200 (1989)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] Y.Sofue; M.Fujimoto; et al.: "Global structures of magnetic field in spiral galaxies" Ann. Rev. Astr. Astrophys.24,. 459-497 (1986)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] Y.Sofue et al.: "The magnetic field near the galactic center" Publ. Astr. Soc. Jpn.39. 95-107 (1987)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] M.Fujimoto et al: "Physical conditions in spiral galaxies and dynamo" Astr. Astrophys.192. 19-29 (1988)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] Y.Sofue; M.Fujimoto: "The vertical large-scale magnetic field in the galactic cen" Publ. Astr. Soc. Jpn.39. 843-848 (1987)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] Y.Sofue et al: "A Galactic Center Jet" Astrophys. J.(1989)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] Y.Sofue: The Radio Universe. Kyoritsu-shuppan K.K., 168 (1988)

    • Description
      「研究成果報告書概要(欧文)」より

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Published: 1990-03-20  

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