时间
发表于 2025-3-21 18:28:43
书目名称How does the Galaxy work?影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0428728<br><br> <br><br>书目名称How does the Galaxy work?影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0428728<br><br> <br><br>书目名称How does the Galaxy work?网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0428728<br><br> <br><br>书目名称How does the Galaxy work?网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0428728<br><br> <br><br>书目名称How does the Galaxy work?被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0428728<br><br> <br><br>书目名称How does the Galaxy work?被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0428728<br><br> <br><br>书目名称How does the Galaxy work?年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0428728<br><br> <br><br>书目名称How does the Galaxy work?年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0428728<br><br> <br><br>书目名称How does the Galaxy work?读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0428728<br><br> <br><br>书目名称How does the Galaxy work?读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0428728<br><br> <br><br>
spinal-stenosis
发表于 2025-3-21 22:13:57
How does the Galaxy work?978-1-4020-2620-1Series ISSN 0067-0057 Series E-ISSN 2214-7985
香料
发表于 2025-3-22 03:47:04
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Lobotomy
发表于 2025-3-22 06:49:06
https://doi.org/10.1007/1-4020-2620-XBulge; Galaxy; Redshift; stars; stellar
名次后缀
发表于 2025-3-22 09:58:46
The Milky Way: Four Centuries of Discovery of the Galaxy,This general introduction is intended to place the present meeting in a broader historical context, highlighting some of the critical junctions in our understanding of the small and large scale structure and evolution of the Galaxy.
output
发表于 2025-3-22 14:13:11
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新字
发表于 2025-3-22 17:31:29
Dark Hydrogen in the Galactic Plane,New high-resolution surveys reveal an abundance of cold H . features in the Galactic plane. These frequently trace spiral arm structure while failing to trace CO features as well as they should if the cold H . is primarily in molecular clouds.
男生如果明白
发表于 2025-3-22 22:42:33
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侧面左右
发表于 2025-3-23 04:20:29
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/h/image/428728.jpg
预定
发表于 2025-3-23 08:16:47
,Brackett-γ Line Survey of the Ionized Hydrogen in the Galactic Plane,ryogenic Fabry-Perot spectrometer. For this survey fields were selected along the Galactic plane from 358° to 43° longitude. The velocity range of the observed emission features ranges from −10 km s. to 90 km s. (LSR). Typical detected intensities correspond to emission measures of about 1000 cm. pc.