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Titlebook: Shocks in Astrophysics; Proceedings of an In T. J. Millar,A. C. Raga Conference proceedings 1995 Kluwer Academic Publishers 1995 Galaxy.Sup

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书目名称Shocks in Astrophysics
副标题Proceedings of an In
编辑T. J. Millar,A. C. Raga
视频video
图书封面Titlebook: Shocks in Astrophysics; Proceedings of an In T. J. Millar,A. C. Raga Conference proceedings 1995 Kluwer Academic Publishers 1995 Galaxy.Sup
描述This volume contains the proceedings of an international conference on Shocks in Astrophysics held at UMIST, Manchester, England from January 9-12, 1995. The study of interstellar and circumstellar gas dynamics has a long and distinguished history in Manchester and has been almost entirely concentrated in the school founded by Franz Kahn in the Astronomy Department, University of Manchester. In January 1993, one of us (AR) was appointed to the faculty of the Astrophysics Group in the Department of Mathematics at UMIST and astrophysical gas dynam­ ics became a major interest of the Group. The subject of this conference was chosen partly for the topicality of the subject matter and partly to help synthesise this expertise with the expertise in interstellar chemistry already present in the Group. The first fruits of this synthesis are contained in this volume. As it happened, this conference celebrated, not so much the beginnings of a long and fruitful collabo­ ration, but rather gave many of Alex‘s friends the chance to say a fond farewell as he departed UMIST at the end of January 1995 to take up a chair at UNAM, Mexico City. The core of this volume consists of twelve review article
出版日期Conference proceedings 1995
关键词Galaxy; Supernova; active galactic nuclei; astrophysics; galaxies; relativistic jet; solar wind; spectrosco
版次1
doihttps://doi.org/10.1007/978-94-009-1624-1
isbn_softcover978-94-010-7225-0
isbn_ebook978-94-009-1624-1
copyrightKluwer Academic Publishers 1995
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https://doi.org/10.1007/978-94-009-1624-1Galaxy; Supernova; active galactic nuclei; astrophysics; galaxies; relativistic jet; solar wind; spectrosco
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978-94-010-7225-0Kluwer Academic Publishers 1995
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H2 in Molecular Shocks: Observations from 2 To 12 Microns,1 (Brand et al. 1988; Parmar et al. 1994) and are consistent with a partially dissociative J-shock. The similarity with Orion suggests the shock processes which dominate the emission in both regions are essentially identical.
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The Importance of Chemical Data for the Study of Interstellar Shocks,e of values of the pre-shock gas density and magnetic induction. The time required to re-establish equilibrium in the post-shock gas depends on the initial conditions and can become very-large. The significance of the two known chemical phases of dark clouds and of bistability is considered in this context.
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Circumstellar Shocks,The presence of shocks in a wide variety of circumstellar phenomena will be illustrated and discussed.
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Ir Observations of Shock Waves in the Interstellar Medium,A description of the development of the use of H. lines as diagnostics of shock excitation in molecular clouds is given. The use of both line ratios and of velocity profiles provides constraints on the models so tight that it may be possible to reject most or even all of the standard stationary shock models.
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