Titlebook: ;

CURD

书目名称Groups of Galaxies in the Nearby Universe影响因子(影响力)




书目名称Groups of Galaxies in the Nearby Universe影响因子(影响力)学科排名




书目名称Groups of Galaxies in the Nearby Universe网络公开度




书目名称Groups of Galaxies in the Nearby Universe网络公开度学科排名




书目名称Groups of Galaxies in the Nearby Universe被引频次




书目名称Groups of Galaxies in the Nearby Universe被引频次学科排名




书目名称Groups of Galaxies in the Nearby Universe年度引用




书目名称Groups of Galaxies in the Nearby Universe年度引用学科排名




书目名称Groups of Galaxies in the Nearby Universe读者反馈




书目名称Groups of Galaxies in the Nearby Universe读者反馈学科排名

遗忘

压倒性胜利

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.

领袖气质

微生物

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.

不如屎壳郎

不如屎壳郎

暂时中止

有斑点

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.

BANAL

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.