Titlebook: How does the Galaxy work?; A Galactic Tertulia Emilio J. Alfaro,Enrique Pérez,José Franco Conference proceedings 2004 Springer Science+Bus

時(shí)間

書目名稱How does the Galaxy work?影響因子(影響力)




書目名稱How does the Galaxy work?影響因子(影響力)學(xué)科排名




書目名稱How does the Galaxy work?網(wǎng)絡(luò)公開度




書目名稱How does the Galaxy work?網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱How does the Galaxy work?被引頻次




書目名稱How does the Galaxy work?被引頻次學(xué)科排名




書目名稱How does the Galaxy work?年度引用




書目名稱How does the Galaxy work?年度引用學(xué)科排名




書目名稱How does the Galaxy work?讀者反饋




書目名稱How does the Galaxy work?讀者反饋學(xué)科排名

spinal-stenosis

How does the Galaxy work?978-1-4020-2620-1Series ISSN 0067-0057 Series E-ISSN 2214-7985

香料

Lobotomy

https://doi.org/10.1007/1-4020-2620-XBulge; Galaxy; Redshift; stars; stellar

名次后綴

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

新字

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

側(cè)面左右

Astrophysics and Space Science Libraryhttp://image.papertrans.cn/h/image/428728.jpg

預(yù)定

,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.