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樓主
發(fā)表于 2025-3-21 17:51:19 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Groups of Galaxies in the Nearby Universe
編輯Ivo Saviane,Valentin D. Ivanov,Jordanka Borissova
視頻videohttp://file.papertrans.cn/390/389004/389004.mp4
叢書名稱ESO Astrophysics Symposia
圖書封面Titlebook: ;
出版日期Conference proceedings 2007
版次1
doihttps://doi.org/10.1007/978-3-540-71173-5
isbn_softcover978-3-642-09026-4
isbn_ebook978-3-540-71173-5Series ISSN 1431-2433 Series E-ISSN 1611-6143
issn_series 1431-2433
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 21:23:18 | 只看該作者
板凳
發(fā)表于 2025-3-22 01:52:53 | 只看該作者
Physical Examination of the Shoulderusing independent distances we will be able to derive Hi mass functions and local star formation densities for the Local Volume as well as nearby galaxy groups such as the CenA and Sculptor groups. A complementary .-band survey will also allow us to analyse the (baryonic) Tully-Fisher relation.
地板
發(fā)表于 2025-3-22 08:14:30 | 只看該作者
5#
發(fā)表于 2025-3-22 11:17:51 | 只看該作者
Reaction kinetics of coordination compounds,iends of Friends algorithm. It is important to stress, however, that there are also important differences, whose discussion could be useful to gain insight on the nature of galaxy groups, and to complement the results of other studies.
6#
發(fā)表于 2025-3-22 16:56:47 | 只看該作者
7#
發(fā)表于 2025-3-22 18:51:59 | 只看該作者
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發(fā)表于 2025-3-22 22:02:59 | 只看該作者
9#
發(fā)表于 2025-3-23 04:57:06 | 只看該作者
Properties of RR Lyrae Stars in the Inner Regions of the Large Magellanic Cloud. II. The Extended SaLMC RR Lyrae, and metallicities for 78 RR Lyrae, nearly tripling the previous sample. These targets are located in 11 fields covering a wide range of distances, out to 2.5 degrees from the center of the LMC. The sample allows us to compare the kinematics of the old and metal-poor stars in the LMC with the rest of the stellar populations.
10#
發(fā)表于 2025-3-23 08:27:46 | 只看該作者
Diffuse Ionized Gas in the Dwarf Galaxy DDO 53 galaxies, the spectral characteristics are very diferent to those of the DIG in spiral galaxies: the excitation is higher and the [SII/Hα] much lower. A combination of leakage photoionization models plus shocks will be able to explain these characteristics.
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