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

只看該作者 · 發(fā)表于 2025-3-21 19:47:38

書(shū)目名稱(chēng)Jets in Young Stellar Objects影響因子(影響力)

書(shū)目名稱(chēng)Jets in Young Stellar Objects影響因子(影響力)學(xué)科排名

書(shū)目名稱(chēng)Jets in Young Stellar Objects網(wǎng)絡(luò)公開(kāi)度

書(shū)目名稱(chēng)Jets in Young Stellar Objects網(wǎng)絡(luò)公開(kāi)度學(xué)科排名

書(shū)目名稱(chēng)Jets in Young Stellar Objects被引頻次

書(shū)目名稱(chēng)Jets in Young Stellar Objects被引頻次學(xué)科排名

書(shū)目名稱(chēng)Jets in Young Stellar Objects年度引用

書(shū)目名稱(chēng)Jets in Young Stellar Objects年度引用學(xué)科排名

書(shū)目名稱(chēng)Jets in Young Stellar Objects讀者反饋

書(shū)目名稱(chēng)Jets in Young Stellar Objects讀者反饋學(xué)科排名

只看該作者 · 發(fā)表于 2025-3-21 23:01:00

只看該作者 · 發(fā)表于 2025-3-22 02:34:07

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

只看該作者 · 發(fā)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.

只看該作者 · 發(fā)表于 2025-3-22 11:05:49

只看該作者 · 發(fā)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

只看該作者 · 發(fā)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

只看該作者 · 發(fā)表于 2025-3-23 00:35:49

只看該作者 · 發(fā)表于 2025-3-23 03:24:32

只看該作者 · 發(fā)表于 2025-3-23 06:06:49

		自動(dòng)登錄	找回密碼
密碼			To register

關(guān)于派博傳思			派博傳思旗下網(wǎng)站			友情鏈接
派博傳思介紹	公司地理位置	論文服務(wù)流程	影響因子官網(wǎng)	吾愛(ài)論文網(wǎng)	大講堂	北京大學(xué)	Oxford Uni.	Harvard Uni.
發(fā)展歷史沿革	期刊點(diǎn)評(píng)	投稿經(jīng)驗(yàn)總結(jié)	SCIENCEGARD	IMPACTFACTOR	派博系數(shù)	清華大學(xué)	Yale Uni.	Stanford Uni.
\|Archiver\|手機(jī)版\|小黑屋\| 派博傳思國(guó)際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-7 17:31
Copyright © 2001-2015 派博傳思京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved