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Titlebook: Jets in Young Stellar Objects; Theory and Observati A. J. L. Fernandes,P. J. V. Garcia,J. J. G. Lima Book 2003 Springer Science+Business Me

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發(fā)表于 2025-3-21 19:47:38 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Jets in Young Stellar Objects
副標(biāo)題Theory and Observati
編輯A. J. L. Fernandes,P. J. V. Garcia,J. J. G. Lima
視頻videohttp://file.papertrans.cn/501/500886/500886.mp4
圖書封面Titlebook: Jets in Young Stellar Objects; Theory and Observati A. J. L. Fernandes,P. J. V. Garcia,J. J. G. Lima Book 2003 Springer Science+Business Me
出版日期Book 2003
關(guān)鍵詞Accretion; accretion disk; active galactic nuclei; black hole; black holes; galaxy; gamma-ray burst; magnet
版次1
doihttps://doi.org/10.1007/978-94-007-0999-7
isbn_softcover978-94-010-3764-8
isbn_ebook978-94-007-0999-7
copyrightSpringer Science+Business Media Dordrecht 2003
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 23:01:00 | 只看該作者
板凳
發(fā)表于 2025-3-22 02:34:07 | 只看該作者
The Structure of Young Stellar Jets and Winds Revealed By High Resolution [Fe Ii] λL.644μM Line Obsediagrams of the [Fe II] λ 1.644 μm emission line revealed remarkably similar characteristics for the two sources, showing two distinct velocity components separated from each other in both velocity and space with the entire emission range blueshifted with respect to the stellar velocity. The high ve
地板
發(fā)表于 2025-3-22 06:29:31 | 只看該作者
Star-Driven Wind and Jet Models-wind models. We emphazise the roles of the magnetic rotator and the disk in the formation and the evolution of the jet. We conjecture that with time both the efficiency of the magnetic rotator and the role of the disk as a primary source for the wind decline.
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發(fā)表于 2025-3-22 11:05:49 | 只看該作者
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發(fā)表于 2025-3-22 16:38:19 | 只看該作者
New Ideas on Jets and Outflows Interactionsng the jet, the molecular outflow is powered by the infailing matter and follows a circulation pattern around the central object without necessarily being entrained by the jet. The model produces a heated pressure-driven outflow with magneto-centrifugal acceleration and collimation. We will try to c
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發(fā)表于 2025-3-22 19:06:26 | 只看該作者
Continuum Excess Emission in Young Low Mass Stars understanding about the CTTS systems impinges directly on our ability to achieve a deeper knowledge of the final stages of low mass stars formation, of the pre-main sequence history of the Sun and even on the processes that lead to planet formation. Here I present a portion of the . of the CTTS sys
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