Titlebook: ;

逢迎春日

多嘴

Environmental Effects on Galaxy Evolution Based on the Sloan Digital Sky Surveyrelation, we have found two characteristic environments where galaxy morphologies change dramatically, indicating there exist two different physical mechanisms responsible for the cluster galaxy evolution. We also found an unusual population of galaxies, which have spiral morphology but do not have

Ordeal

The Low-luminosity Galaxy Population in the NGC 5044 Groupong objects originally classified as early-type dwarfs. Particularly, a significant fraction of bright dwarf “ellipticals” show a distinct bulge+disc structure; we thus re-classify these objects as dwarf lenticulars (dS0).

gnarled

出汗

編輯才信任

https://doi.org/10.1007/978-94-009-9992-3ope and the Australia Telescope Compact Array to produce a census of all the gas-rich galaxies and potential analogs to the high-velocity clouds (HVCs) within these groups down to M. ≤ 10.M.as a test of models of galaxy formation. We present the HI mass function and halo mass function for these anal

自作多情

Spectral Lines of Atmospheric Gases,ield and 13 in the clusters NGC1835 and NGC2019. 15 RR Lyrae stars of .Cen were observed as well for comparison. We measured radial velocities for 87 LMC 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

Debate

有罪

Infirm