A study of the regular structure of the galactic magnetic field using WMAP5 polarization data at 22 GHz
We study the spatial structure of the 3-dimensional large-scale pattern of the Galactic Magnetic Field using the polarization maps obtained by the WMAP...
A study of the wind of P Cygni applying the self-absorption-curve method
After a brief description of how spectral emission lines can be studied by the self-absorption-curve method, we show what happens when it is used to examine the...
We present the first deep, optical, wide-field imaging survey of the young open cluster Collinder 359, complemented by near-infrared follow-up observations...
A Study on the Kinematics of the HII Regions of NGC 4449
We have used the TAURUS Fabry-Perot imaging spectrograph at the William Hershell Telescope of the Observatorio del Roque de los Muchachos to study the...
A suite of community tools for spectro-polarimetric analysis .
The National Center for Atmospheric Research (NCAR) has undertaken a 3-year initiative to develop the Community Spectro-polarimetric Analysis Center (CSAC). The...