Researcher and Associate Professor at the Astrophysics Department (GUAIX group), in the Universidad Complutense de Madrid (UCM).
Contact
Departamento de Astrofísica y Ciencias de la Atmósfera
Facultad de Ciencias Físicas
Avda. Complutense s/n
28040, Madrid (Spain)
Telf.: (+34) 91 3945179
Fax: (+34) 91 3944635
e-mail: acasmor([at] fis.ucm.es)
Curriculum
Nuclear spectrum of NGC 4321 with the
   stellar template plotted on top in red line. The inner panel shows
   in detail the fit of the Na D absorption doublet (red line) and the
   residuals (blue line). X-ray image of the central (32 arcsec)2 of the clus- 
ter RBS797. There are clear minima in the X-ray emission 
in ENE and WSW direction at about 5 arcseconds from 
the cluster centre (see arrows). An excess of emission is 
found in perpendicular directions.