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Frida:diffraction limited imaging and integral field spectroscopy with gtc。
A Simple Model for Hydromagnetic Instabilities in the Presence of a Constant Magnetic Field
The EROs at z < 1.5 in the Groth-Westphal field of the GOYA survey     The EROs  Groth-Westphal field  z < 1.5  GOYA survey       font style='font-size:12px;'> 2009/6/25
The EROs at z < 1.5 in the Groth-Westphal field of the GOYA survey。
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
The Lifetimes of Molecular Cloud Cores:What is the Role of the Magnetic Field?
Galaxy Formation Simulations with Scalar Field Dark Matter。
The present article has systematically solved the problem of galaxy formation and some significant cosmological puzzles. First a mistake with Einstein’s equation of gravitational field is corrected, n...
Small field CCD astrometry with a long focus reflector telescope     CCD astrometry  reflector telescope       font style='font-size:12px;'> 2009/6/11
Small field CCD astrometry with a long focus reflector telescope。
Azimuthal field perturbations in the jovian magnetosphere:ulysses observations。
New estimations of the relation between the alpha-effect and magnetic field fluctuations
Collapse and fragmentation models of cloud cores with magnetic field support。
Magnetic field topology in jets     Magnetic field topology  radiative jet       font style='font-size:12px;'> 2009/6/4
We present results on the magnetic field topology in a pulsed radiative jet.For initially helical magnetic fields and perio dic velo city variations, we find thatthe magnetic field alternates along th...
Evaluation by Numerical Simulations of the Block Adjustment Method in Small Field CCD Astrometry
The concept that open magnetic flux of the Sun (rooted with one and only one footpoint at the Sun) is a conserved quantity is taking root in the heliospheric community. Observations show that the Sun'...
We analyse different observational data related to the problem of intrinsic magnetic field strength in small-scale fluxtubes outside sunspots. We conclude that the kG range of fluxtube fields follow...

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