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Observations of jets in H II regions (hh 444)     jets  H II regions        font style='font-size:12px;'> 2009/6/5
Observations of jets in H II regions (hh 444)。
Oxygen and helium abundances in galactic h II regions:abundance gradients     h II regions  Oxygen  helium       font style='font-size:12px;'> 2009/6/5
Oxygen and helium abundances in galactic h II regions:abundance gradients。
Effects of the stellar component on derived physical parameters of galactic H II regions
The effects of dust and density distributions in uc H II regions
U ltracompact H II regions:new challenges     H II regions  lower electron density       font style='font-size:12px;'> 2009/6/5
U ltracompact H II regions:new challenges
Photoionization models for giant h ii regions     Photoionization models  h ii regions  WOLF-RAYET       font style='font-size:12px;'> 2009/6/5
Photoionization models for giant h ii regions
Cloudy 94 and applications to quasar emission line regions     quasar emission line regions  Cloudy 94       font style='font-size:12px;'> 2009/6/5
Cloudy 94 and applications to quasar emission line regions
We review some recent results of three-dimensional smoothed particle hydro-dynamics (SPH) simulations of overdense, radiatively cooling jets in star formingregions. We discuss the structure and kinema...
Three Galactic star forming regions associated with W3(OH), S209 and S187 have been simultaneously mapped in two trans-IRAS far infrared (FIR) bands centered at 140 and 200m using the TIFR 100 cm ...
If subduction zone earthquakes conform to a characteristic model, in which persistent segments fail at predictable stress levels due to the steady accumulation of tectonic loading, historical seismici...
To interpret the millimeter and sub-millimeter line emissions of atomic and molecular species from galactic and extragalactic photodissociation regions, warm gas components and molecular clouds, gen...
The paper extends the Representative Elementary Watershed (REW) theory for cold regions through explicit treatment of energy balance equations to include associated processes and process descriptions....
The interaction between vegetation and hydrologic processes is particularly tight in water-limited environments where a positive-feedback links soil moisture and vegetation. The vegetation of these sy...
Magnetic Source Regions of Coronal Mass Ejections      Coronal mass ejection  flare  filament eruption       font style='font-size:12px;'> 2009/5/7
The majority of flare activity arises in active regions which contain sunspots, while Coronal Mass Ejection (CME) activity can also originate from decaying active regions and even so-called quiet sola...
Helicity of Solar Active Regions from a Dynamo Model     MHD  Sun:activity  Sun:magnetic fields  sunspots       font style='font-size:12px;'> 2009/5/7
We calculate helicities of solar active regions based on the idea that poloidal flux lines get wrapped around a toroidal flux tube rising through the convection zone, thereby giving rise to the helici...

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