Croching
发表于 2025-3-21 19:47:38
书目名称Jets in Young Stellar Objects影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0500886<br><br> <br><br>书目名称Jets in Young Stellar Objects影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0500886<br><br> <br><br>书目名称Jets in Young Stellar Objects网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0500886<br><br> <br><br>书目名称Jets in Young Stellar Objects网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0500886<br><br> <br><br>书目名称Jets in Young Stellar Objects被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0500886<br><br> <br><br>书目名称Jets in Young Stellar Objects被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0500886<br><br> <br><br>书目名称Jets in Young Stellar Objects年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0500886<br><br> <br><br>书目名称Jets in Young Stellar Objects年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0500886<br><br> <br><br>书目名称Jets in Young Stellar Objects读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0500886<br><br> <br><br>书目名称Jets in Young Stellar Objects读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0500886<br><br> <br><br>
Demonstrate
发表于 2025-3-21 23:01:00
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删除
发表于 2025-3-22 02:34:07
The Structure of Young Stellar Jets and Winds Revealed By High Resolution λL.644μM Line Obsediagrams of the 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
搜集
发表于 2025-3-22 06:29:31
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.
SLUMP
发表于 2025-3-22 11:05:49
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Kidney-Failure
发表于 2025-3-22 16:38:19
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
Evolve
发表于 2025-3-22 19:06:26
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
Dendritic-Cells
发表于 2025-3-23 00:35:49
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昏暗
发表于 2025-3-23 03:24:32
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缩短
发表于 2025-3-23 06:06:49
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