到来
发表于 2025-3-21 16:06:16
书目名称Highlights of Spanish Astrophysics IV影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0427027<br><br> <br><br>书目名称Highlights of Spanish Astrophysics IV影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0427027<br><br> <br><br>书目名称Highlights of Spanish Astrophysics IV网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0427027<br><br> <br><br>书目名称Highlights of Spanish Astrophysics IV网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0427027<br><br> <br><br>书目名称Highlights of Spanish Astrophysics IV被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0427027<br><br> <br><br>书目名称Highlights of Spanish Astrophysics IV被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0427027<br><br> <br><br>书目名称Highlights of Spanish Astrophysics IV年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0427027<br><br> <br><br>书目名称Highlights of Spanish Astrophysics IV年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0427027<br><br> <br><br>书目名称Highlights of Spanish Astrophysics IV读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0427027<br><br> <br><br>书目名称Highlights of Spanish Astrophysics IV读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0427027<br><br> <br><br>
Concomitant
发表于 2025-3-21 23:45:56
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协议
发表于 2025-3-22 02:05:01
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FOIL
发表于 2025-3-22 04:48:47
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Anecdote
发表于 2025-3-22 10:02:25
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GLARE
发表于 2025-3-22 13:06:17
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取之不竭
发表于 2025-3-22 19:36:28
OSIRIS: Status and Sciencefield of view, and capabilities for direct imaging, both long-slit and multiple object spectroscopy, and fast spectrophotometry. The combination of OSIRIS wide field, tunable filters plus charge shuffling array detectors, will constitute the most powerful instrument for studying faint emission-line
头脑冷静
发表于 2025-3-22 22:53:20
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lethal
发表于 2025-3-23 05:07:00
The Star Formation History of Early-type Galaxies as a Function of Environmentronments. Using new models, that include a new and improved stellar library, we derive mean ages, metallicities and study the qualitative behaviour of different chemical elements. We conclude that more massive galaxies formed their stars on shorter time-scales than less massive ones. The formation e
RLS898
发表于 2025-3-23 08:56:58
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