Tyler
发表于 2025-3-21 17:19:23
书目名称Galaxies and their Masks影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0380353<br><br> <br><br>书目名称Galaxies and their Masks影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0380353<br><br> <br><br>书目名称Galaxies and their Masks网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0380353<br><br> <br><br>书目名称Galaxies and their Masks网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0380353<br><br> <br><br>书目名称Galaxies and their Masks被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0380353<br><br> <br><br>书目名称Galaxies and their Masks被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0380353<br><br> <br><br>书目名称Galaxies and their Masks年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0380353<br><br> <br><br>书目名称Galaxies and their Masks年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0380353<br><br> <br><br>书目名称Galaxies and their Masks读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0380353<br><br> <br><br>书目名称Galaxies and their Masks读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0380353<br><br> <br><br>
Banquet
发表于 2025-3-21 22:02:54
Kenneth Lyons Jones,H. Eugene Hoymeuch as rings, nuclear arms, nuclear bars, and asymmetries. We find a centrally peaked concentration in about 85% of the galaxies with typical size scales of about 0.5–1 kpc. This might be related to perturbations produced by recent interactions.
情节剧
发表于 2025-3-22 01:11:56
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飞行员
发表于 2025-3-22 06:38:02
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使虚弱
发表于 2025-3-22 10:12:54
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LEERY
发表于 2025-3-22 16:12:43
Sonal,Sharmita Gupta,Yati Prabha,S. K. Sonillicity gradient, bars with null metallicity gradient, and galaxies with positive metallicity gradient. Regarding the bulge region we find that the ages and metallicities are younger and more metal rich, at a given ., than the bulges of unbarred galaxies. The bulges of the barred galaxies in our sam
LEERY
发表于 2025-3-22 17:15:21
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obeisance
发表于 2025-3-23 01:04:11
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组成
发表于 2025-3-23 04:43:28
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PHIL
发表于 2025-3-23 08:05:31
The Large Magellanic Cloud: A Power Spectral Analysis of Spitzer Images,similar to the in-plane velocities at small scales. The motions are highly anisotropic at large scales,with in-plane velocities being much more important than vertical ones.In contrast, at small scales, the motions become more isotropic.