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近日,山东大学威海校区石维彬副教授等人通过分析LAMOST K巨星数据与SDSS RGB数据确认了一个已知分支,并在人马矮星系Leading星流上证认了一个新分支。这个新分支有助于限制人马矮星系星流的子结构和银河系势能。此成果已发表在国际知名天文期刊“Astronomy & Astrophysics”(A&A,2017, 597, A54)上。
We investigate the incidence of major mergers creating massive (Mstar > 1011 M⊙) galaxies in present-day (z≤ 0.12) groups and clusters. Using a volume-limited sample of 845 groups with dark matter hal...
Most massive galaxies contain supermassive black holes (SMBHs) in their cores. When galaxies merge, gas is driven to nuclear regions and can accrete onto the central black hole. Thus one expects to se...
We show that the distribution of luminosities of Brightest Cluster Galaxies, in two SDSS-based group catalogs, suggests that BCG luminosities are just the statistical extremes of the group galaxy lumi...
Taking into account a range of parameters determined from the evolutionary models and available observational data, the detailed non-LTE spectra for the primary star and the irradiated donor star in t...
The quasar SDSS J133401.39+331534.3 at z = 2.426 is found to be a two-image gravitationally lensed quasar with the image separation of 0.833. The object is first identified as a lensed quasar candidat...
Characterization of Isolated Galaxies in the Local Universe from SDSS (DR5)。
Attenuation curves (laws) in the optical part of the spectrum (from about 3500 ºA to 9000 ºA) are determined for galaxies with di®erent star formation histories (SFHs) using images in &m...

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