找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

Titlebook: CO: Twenty-Five Years of Millimeter-Wave Spectroscopy; Proceedings of the 1 William B. Latter,Simon J. E. Radford,John Bally Conference pro

[復制鏈接]
查看: 9191|回復: 46
樓主
發(fā)表于 2025-3-21 16:20:50 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy
副標題Proceedings of the 1
編輯William B. Latter,Simon J. E. Radford,John Bally
視頻videohttp://file.papertrans.cn/221/220410/220410.mp4
叢書名稱International Astronomical Union Symposia
圖書封面Titlebook: CO: Twenty-Five Years of Millimeter-Wave Spectroscopy; Proceedings of the 1 William B. Latter,Simon J. E. Radford,John Bally Conference pro
描述Interstellar carbon monoxide (CO) was first detected in 1970 with the 36 foot diameter telescope of the National Radio Astronomy Observatory! on Kitt Peak in Southern Arizona. R. W. Wilson, K. B. Jefferts, and A. A. Penzias of Bell Labs reported, "We have found intense 2.6 mm line radiation 2 from nine Galactic sources which we attribute to carbon monoxide." Soon afterward, several other basic molecules were also observed in space. IAU Symposium 170, CO: Twenty Five Years of Millimeter Wave Spectroscopy, was organized to commemorate those discoveries. The Symposium reviewed the accomplishments of a quarter century of research on interstellar molec- ular gas, surveyed the current state of millimeter-wave spectroscopy, and gave a glimpse of what the next 25 years might hold. Studies of interstellar CO have revolutionized our understanding of the phases and dynamics of the interstellar medium, the initial and final stages of stellar evolution, the chemistry of dense and diffuse interstellar matter and of the solar system, the structure of the Milky Way galaxy, and the content and structure of other galaxies, some very distant. Spectroscopic studies of CO and other molecules are primar
出版日期Conference proceedings 1997
關(guān)鍵詞astronomy; astrophysics; galaxy; interstellar matter; milky way; observatory; planet; radio astronomy; solar
版次1
doihttps://doi.org/10.1007/978-94-011-5414-7
isbn_softcover978-0-7923-4284-7
isbn_ebook978-94-011-5414-7Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightSpringer Science+Business Media Dordrecht 1997
The information of publication is updating

書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy影響因子(影響力)




書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy影響因子(影響力)學科排名




書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy網(wǎng)絡(luò)公開度




書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy網(wǎng)絡(luò)公開度學科排名




書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy被引頻次




書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy被引頻次學科排名




書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy年度引用




書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy年度引用學科排名




書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy讀者反饋




書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy讀者反饋學科排名




單選投票, 共有 1 人參與投票
 

0票 0.00%

Perfect with Aesthetics

 

1票 100.00%

Better Implies Difficulty

 

0票 0.00%

Good and Satisfactory

 

0票 0.00%

Adverse Performance

 

0票 0.00%

Disdainful Garbage

您所在的用戶組沒有投票權(quán)限
沙發(fā)
發(fā)表于 2025-3-21 22:55:19 | 只看該作者
板凳
發(fā)表于 2025-3-22 01:03:58 | 只看該作者
地板
發(fā)表于 2025-3-22 05:47:57 | 只看該作者
5#
發(fā)表于 2025-3-22 12:33:00 | 只看該作者
6#
發(fā)表于 2025-3-22 14:57:12 | 只看該作者
7#
發(fā)表于 2025-3-22 18:26:15 | 只看該作者
A Molecular Worm in Scutumrvations have so far been confined mainly to several vertical strips across the plane covering a few degrees in Galactic longitude and 6°‐8° in Galactic latitude; details of this on-going survey are given in Dame & Thaddeus (1995).
8#
發(fā)表于 2025-3-22 21:45:21 | 只看該作者
On the Fractal Structure of Molecular Cloudsmportant to study the power spectrum of observed cloud images. For HI clouds (Green 1993), the azimuthally averaged power spectra derived directly from interferometer observations are well characterized by a power law with a spectral index close to 2.8.
9#
發(fā)表于 2025-3-23 03:28:31 | 只看該作者
10#
發(fā)表于 2025-3-23 06:13:49 | 只看該作者
https://doi.org/10.1007/978-3-319-59957-1sed to determine the CR density and calibrate the CO line as a tracer of molecular mass. Dominant production mechanisms for γ rays of energies ~30 MeV-30 GeV are the decay of pions produced in collisions of CR protons with ambient matter and Bremsstrahlung scattering of CR electrons.
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學 Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經(jīng)驗總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學 Yale Uni. Stanford Uni.
QQ|Archiver|手機版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2026-1-29 19:44
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復 返回頂部 返回列表
依安县| 东乌| 汉寿县| 思南县| 吐鲁番市| 郁南县| 德庆县| 大埔县| 东乡| 云南省| 井研县| 遂平县| 永春县| 临夏县| 海南省| 井陉县| 元氏县| 涿鹿县| 自贡市| 云和县| 灌阳县| 宜兰市| 广东省| 巴马| 嘉黎县| 克山县| 苏尼特右旗| 进贤县| 武威市| 兴义市| 江油市| 汾西县| 竹山县| 泉州市| 高淳县| 长沙市| 明星| 通河县| 即墨市| 鲁甸县| 斗六市|