Evolution of a Rotating Protostar

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概要

• 論文の詳細を見る

• A theory of a rotating uniform gas cloud that contracts gravitationally due to secular loss of angular momentum is applied to (Pop. I) protostars of hypothetical origin in the interstellar medium. Representative thermal histories are displayed and the influence of various parameters discussed. It appears that some protostars, particularly the more massive ones, are apt to approach the mainsequence by a Helmholtz-Kelvin-like expansion from below rather than by the familiar contraction from above.

• 1966-04-25

著者

• Bird Joseph

  Applied Physics Laboratory The Johns Hopkins University

• BIRD Joseph

  Applied Physics Laboratory, The Johns Hopkins University

• Bird J.F.

  Applied Physics Laboratory, The Johns Hopkins University

関連論文

• Evolution of a Rotating Protostar

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