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2001 Fiscal Year Final Research Report Summary

Mecanism of Outflow form Dynamically Contracting Molecular Cores

Research Project

Project/Area Number 11640231
Research Category

Grant-in-Aid for Scientific Research (C)

Allocation TypeSingle-year Grants
Section一般
Research Field Astronomy
Research InstitutionNational Astronomical Observatory Of Japam (2000-2001)
Niigata University (1999)

Principal Investigator

TOMISAKA Kohji  National Astronomical Observatory Of Japam theoretical Astrophysics Divisiom Professor, 理論天文学研究系, 教授 (70183879)

Co-Investigator(Kenkyū-buntansha) NAKAMURA Fumitaka  Faculty of Education and Human Sciences,Niigata University Department of Physics,Associate Professor, 教育人間科学部, 助教授 (20291354)
Project Period (FY) 1999 – 2001
KeywordsInterstellar Molecular Clouds / Star Formation / Outflow / Dynamical Cotraction / Nested Grid Method / Self-Similar Evolutions
Research Abstract

Dynamical contraction of interstellar molecular clouds is studied. 1. Tomisaka studied the mechanism of molecular outflow with the nested-grid axi-symmetric magnetohydrodynamical simulations. Rotations of the molecular cloud cores amplify the toroidal magnetic fields, which eject the gas as molecular outflows. From the simulations, we explored the followings : (1) Initial rotation speed specifies the epoch when the molecular outflow begins. That is, increasing the angular momentum, the outflow is launched immediate after the adiabatic core is formed. (2) When the initial poloidal magnetic field is strong (its energy is comparable to the thermal one), a U-shaped outflow is formed, in which gas is mainly outflowing through a region whose shape looks like a capital letter U at a finite distance from the rotation axis. (3) The other is a turbulent outflow in which magnetic field lines and velocity fields seem to be randomly oriented, which is realized when the initial magnetic energy is much smaller than the thermal one. In this case, globally the gas moves out almost perpendicularly from the disk and the outflow looks like a capital letter I. 2. Nakamura studied the gravitational collapse of a cloud supported by strong magnetic fields taking into account of the magnetic diffusion. (1) A model with large mass leads to fragmentation to a number of high-densitycores in the early phase. This corresponds to a cluster forming mode. (2) Incontrast, in a less massive cloud a bar grows and the bar breaks into fragments. In this case a binary system will appear.

  • Research Products

    (16 results)

All Other

All Publications (16 results)

  • [Publications] K.Tomisaka: "Outflow from YSO and Angular Momentum Transfer"in "Proceedings of the IAU Symposium on "The Formation of Binary Stars". 401-405 (2001)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] K.Tomisaka: "The Evolution of the Angular Momentum Distribution during Star Formation"Astrophysical Journal (Letters). 528. L41-L44 (2000)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] K.Tomisaka: "Outflows from YSO's and the Angular Momentum of New-Born Stars"in "Star Formation from the Small to the Large Scale". 141-148 (2000)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] K.Tomisaka: "Collapse-Driven Outflow in Star-Forming Molecular Cores"in "Star Formation 1999". 197-198 (2000)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] S.Ogino, K.Tomisaka, F.Nakamura: "Gravitational Collapse of Spherical Isothermal Clouds"Publ. Astron. Soc. Japan. 51. 637-651 (1999)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] F.Nakamura: "Formation of an Infalling Disklike Envelope around a Protostar"The Astrophysical Journal. 543. 291-298 (2000)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] F.Nakamura, Zhi-Yun Li: "Nonaxisymmetric Evolution of Magnetically Subcritical Clouds : Bar Growth, Core Elongation, and Binary Formation"The Astrophysical Journal. 566. L101-L104 (2002)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] 編 S.M.Miyama, K.Tomisaka, T.Hanawa: "Numerical Astrophysics"Kluwer Academic Publishers. 437 (1999)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] K. Tomisaka: "Outflow from YSO and Angular Momentum Transfer in Proceedings of the IAU Simposium"The Formation of Binary Stars. 401-405 (2001)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] K. Tomisaka: "The Evolution of the Angular Momentum Distribution during Star Formation"Astrophysical Journal (Letters). 528. L41-L44 (2000)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] K. Tomisaka: "Outflows from YSO's and the Angular Momentum of New-Born Stars"Star Formation from the Small to the Large Scala. 141-148 (2000)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] K. Tomisaka: "Collapse-Driven Outflow in Star-Forming JtoJecular Cores"Star Formation 1999. 197-198 (2000)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] S. Ogino, K Tomisaka, and F. Nakamura: "Gravitational Collapse of Spherical Isothermal Clouds"Publ. Astron. Soc. Japan. 51. 637-651 (1999)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] F. Nakamura: "Formation of an Mailing Diskiike Envelope around a Protostar"The Astrophysical Journal. 543. 291-298 (2000)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] F. Nakamura and Zhi-Yun Li: "Nonaxisymmetric Evolution of Magnetically Subcritical Clouds : Bar Growth, Core Elongation, and Binary Formation"The Astrophysical Journal. 566. L101-L104 (2002)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] S. M Miyama, K Tomisaka, & T. Hanawa: "Numerical Astrophysics"Kluwer Academic Publishers. 437 (1999)

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

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Published: 2003-09-17  

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