传家宝
发表于 2025-3-21 16:54:20
书目名称Dust-Gas Instabilities in Protoplanetary Disks影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0283450<br><br> <br><br>书目名称Dust-Gas Instabilities in Protoplanetary Disks影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0283450<br><br> <br><br>书目名称Dust-Gas Instabilities in Protoplanetary Disks网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0283450<br><br> <br><br>书目名称Dust-Gas Instabilities in Protoplanetary Disks网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0283450<br><br> <br><br>书目名称Dust-Gas Instabilities in Protoplanetary Disks被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0283450<br><br> <br><br>书目名称Dust-Gas Instabilities in Protoplanetary Disks被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0283450<br><br> <br><br>书目名称Dust-Gas Instabilities in Protoplanetary Disks年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0283450<br><br> <br><br>书目名称Dust-Gas Instabilities in Protoplanetary Disks年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0283450<br><br> <br><br>书目名称Dust-Gas Instabilities in Protoplanetary Disks读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0283450<br><br> <br><br>书目名称Dust-Gas Instabilities in Protoplanetary Disks读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0283450<br><br> <br><br>
织布机
发表于 2025-3-21 22:27:44
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反抗者
发表于 2025-3-22 01:03:42
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生意行为
发表于 2025-3-22 07:06:49
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幻想
发表于 2025-3-22 09:59:14
Mariya Petrova,Seth J. Schwartzt radial drift. The contents of this chapter are based on our published paper: Tominaga et al. (2019), ApJ, 881, 53, DOI: 10.3847/1538-4357/ab25ea. Figures and some texts are reproduced in this thesis with permission from American Astronomical Society (©AAS)
BRUNT
发表于 2025-3-22 15:45:24
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BRUNT
发表于 2025-3-22 17:38:22
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解冻
发表于 2025-3-23 00:27:07
Introduction,ow in size through mutual sticking and form building blocks of planets called planetesimals. Further coalescence of planetesimals leads to formation of planets. However, it is known that there are some barriers against dust growth to planetesimals, and the formation process of planetesimals is still
重画只能放弃
发表于 2025-3-23 04:03:03
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起来了
发表于 2025-3-23 06:12:44
Numerical Simulations of Secular Instabilities,erstand subsequent planetesimal formation. Because of the slow growth of the instability, one has to use numerical methods that are less diffusive and avoid numerical errors as much as possible. Motivated by this, we first formulate Lagrange-cell method for long-term hydrodynamic simulations. Our me