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The field of Loden 112     field  Loden  spatially correlated       font style='font-size:12px;'> 2011/10/12
Based on the available uvbybeta photometry of OB stars in the longitude range 281 - 285 deg in the Galactic disk, we identify a feature of young stars at 1630+/-82 pc, that is probably connected to th...
New Constraints on the Primordial Magnetic Field     primordial magnetic field  numerical analysis       font style='font-size:12px;'> 2010/3/19
We present the newest statistical and numerical analysis of the matter and cosmic microwave background power spectrum with effects of the primordial magnetic field (PMF) included. New limits to the PM...
We present new analysis of the birth rate of AXPs and SGRS and their associated SNRs. Using Kolmogorov-Smirnov statistics together with parametric fits based on a robust estimator, we find a birth rat...
Flat central density profiles from scalar field dark matter halos。
Near-field cosmology with horizontal branch and rr lyrae stars。
Massive Stars in Clusters and the Field     Massive Stars  Clusters  the Field       font style='font-size:12px;'> 2009/6/16
Massive Stars in Clusters and the Field

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