叛乱分子
发表于 2025-3-21 18:25:09
书目名称Dense Molecular Gas around Protostars and in Galactic Nuclei影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0265606<br><br> <br><br>书目名称Dense Molecular Gas around Protostars and in Galactic Nuclei影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0265606<br><br> <br><br>书目名称Dense Molecular Gas around Protostars and in Galactic Nuclei网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0265606<br><br> <br><br>书目名称Dense Molecular Gas around Protostars and in Galactic Nuclei网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0265606<br><br> <br><br>书目名称Dense Molecular Gas around Protostars and in Galactic Nuclei被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0265606<br><br> <br><br>书目名称Dense Molecular Gas around Protostars and in Galactic Nuclei被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0265606<br><br> <br><br>书目名称Dense Molecular Gas around Protostars and in Galactic Nuclei年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0265606<br><br> <br><br>书目名称Dense Molecular Gas around Protostars and in Galactic Nuclei年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0265606<br><br> <br><br>书目名称Dense Molecular Gas around Protostars and in Galactic Nuclei读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0265606<br><br> <br><br>书目名称Dense Molecular Gas around Protostars and in Galactic Nuclei读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0265606<br><br> <br><br>
Blatant
发表于 2025-3-21 21:23:03
Domain-Specific Languages in Practiceeakage for the evolution of cloud cores; (iii) the phase of anisotropic dynamical collapse following the formation of strongly peaked density distributions; (iv) the mechanism of magnetic braking as a possible solution to the angular momentum problem in star formation.
ELATE
发表于 2025-3-22 00:30:57
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沉思的鱼
发表于 2025-3-22 07:56:57
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尾巴
发表于 2025-3-22 09:55:26
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exophthalmos
发表于 2025-3-22 12:55:56
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exophthalmos
发表于 2025-3-22 17:54:23
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战役
发表于 2025-3-22 22:09:36
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nerve-sparing
发表于 2025-3-23 02:35:28
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啤酒
发表于 2025-3-23 08:44:18
Magnetic Fields in Star-Forming Regions: Theoretical Aspectseakage for the evolution of cloud cores; (iii) the phase of anisotropic dynamical collapse following the formation of strongly peaked density distributions; (iv) the mechanism of magnetic braking as a possible solution to the angular momentum problem in star formation.