HEIR
发表于 2025-3-21 17:03:03
书目名称A Statistical and Multi-wavelength Study of Star Formation in Galaxies影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0142261<br><br> <br><br>书目名称A Statistical and Multi-wavelength Study of Star Formation in Galaxies影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0142261<br><br> <br><br>书目名称A Statistical and Multi-wavelength Study of Star Formation in Galaxies网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0142261<br><br> <br><br>书目名称A Statistical and Multi-wavelength Study of Star Formation in Galaxies网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0142261<br><br> <br><br>书目名称A Statistical and Multi-wavelength Study of Star Formation in Galaxies被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0142261<br><br> <br><br>书目名称A Statistical and Multi-wavelength Study of Star Formation in Galaxies被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0142261<br><br> <br><br>书目名称A Statistical and Multi-wavelength Study of Star Formation in Galaxies年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0142261<br><br> <br><br>书目名称A Statistical and Multi-wavelength Study of Star Formation in Galaxies年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0142261<br><br> <br><br>书目名称A Statistical and Multi-wavelength Study of Star Formation in Galaxies读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0142261<br><br> <br><br>书目名称A Statistical and Multi-wavelength Study of Star Formation in Galaxies读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0142261<br><br> <br><br>
许可
发表于 2025-3-21 22:51:11
https://doi.org/10.1007/978-3-662-61122-7in a regime that could not be probed by the . satellite. At all . and at least for ., I measured the dispersion of .s around this relation and found it to be relatively small, reinforcing the idea that the majority of the star formation in the Universe is happening through a steady, secular process that has yet to be clearly identified.
争吵
发表于 2025-3-22 04:06:23
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一美元
发表于 2025-3-22 05:16:09
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先兆
发表于 2025-3-22 11:56:05
Die Angst ohne wirkliche Gefahr.); and second, the mass fraction of PAH molecules is a free parameter, allowing a finer modeling of the MIR photometry around .. This last point will be particularly important in the . (.) era, when we will routinely observe galaxies in deep MIR surveys.
irreparable
发表于 2025-3-22 13:29:21
Die Angst ohne wirkliche GefahrIn this chapter I present an analysis of the deepest . images in four major extragalactic fields: GOODS–North, GOODS–South, UDS, and COSMOS.
EWE
发表于 2025-3-22 20:27:19
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注意力集中
发表于 2025-3-22 22:25:11
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cardiac-arrest
发表于 2025-3-23 01:24:45
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不适
发表于 2025-3-23 06:36:21
Die Angst ohne wirkliche Gefahrlation between the . and the stellar mass (.) (a.k.a. the Main Sequence) of a mass-complete sample of galaxies, I found that the slope of the correlation was evolving with both redshift and stellar mass.