Dopamine
发表于 2025-3-21 20:04:49
书目名称Seminar on Concurrency影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0864950<br><br> <br><br>书目名称Seminar on Concurrency影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0864950<br><br> <br><br>书目名称Seminar on Concurrency网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0864950<br><br> <br><br>书目名称Seminar on Concurrency网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0864950<br><br> <br><br>书目名称Seminar on Concurrency被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0864950<br><br> <br><br>书目名称Seminar on Concurrency被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0864950<br><br> <br><br>书目名称Seminar on Concurrency年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0864950<br><br> <br><br>书目名称Seminar on Concurrency年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0864950<br><br> <br><br>书目名称Seminar on Concurrency读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0864950<br><br> <br><br>书目名称Seminar on Concurrency读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0864950<br><br> <br><br>
新星
发表于 2025-3-21 21:28:25
http://reply.papertrans.cn/87/8650/864950/864950_2.png
草本植物
发表于 2025-3-22 01:39:47
http://reply.papertrans.cn/87/8650/864950/864950_3.png
GLOOM
发表于 2025-3-22 04:52:02
Glynn Winskelccurred within the domains of astronomical observations, astrophysical modeling and numerical simulations, but the recent advent of high energy density facilities has added experimental control to jet studies...Front-line research on jet launching and collimation requires a highly interdisciplinary
易于
发表于 2025-3-22 10:41:28
J. A. Bergstra,J. W. Klop,J. V. Tucker in the introduction, this reflects very much the quite different mode of energy transport in the two classes of source. Another parameter which also highlights the differences between the two types of jet is the velocity. This can be written in the form: .. = 430 km s...... (./..)...For class I jet
抛射物
发表于 2025-3-22 13:50:37
J. Misraspeed, density, magnetic fields, collimation) must be related in a way to the properties of the very central object and its accretion disk. Early models of jet formation were based on pure hydrodynamic acceleration in the funnels of geometrically thick tori. For sub-Eddington luminosities such flows
不溶解
发表于 2025-3-22 18:41:44
Ben Moszkowskispeed, density, magnetic fields, collimation) must be related in a way to the properties of the very central object and its accretion disk. Early models of jet formation were based on pure hydrodynamic acceleration in the funnels of geometrically thick tori. For sub-Eddington luminosities such flows
Costume
发表于 2025-3-23 01:03:48
Christian Lengauer,Chua-Huang Huang in the introduction, this reflects very much the quite different mode of energy transport in the two classes of source. Another parameter which also highlights the differences between the two types of jet is the velocity. This can be written in the form: .. = 430 km s...... (./..)...For class I jet
Endemic
发表于 2025-3-23 03:38:39
Gul Aghans. The simulations follow several 1000 Keplerian periods of the inner disk (for animated movies see http : / /www. aip. de/∼cf endt). Our model prescribes a Keplerian disk around a rotating star as a fixed boundary condition. The initial magnetic field distribution remains frozen into the star and
hypnotic
发表于 2025-3-23 06:30:11
Vaughan Prattns. The simulations follow several 1000 Keplerian periods of the inner disk (for animated movies see http : / /www. aip. de/∼cf endt). Our model prescribes a Keplerian disk around a rotating star as a fixed boundary condition. The initial magnetic field distribution remains frozen into the star and