One of the most useful diagnostic tools for the detection of inclined magnetic fields in solar chromospheric and coronal structures is that based on the fact...
A major step in understanding the X-ray generation in comets: recent progress obtained with XMM-Newton
The observation of comet C/2000 WM1 (LINEAR) with XMM-Newton is a highlight in the field of cometary research. During 17 hours of almost uninterrupted...
A map-making algorithm for the QUIJOTE CMB experiment
In the last years we obtained a very detailed picture of the Primordial Universe by, among other means, measuring the intensity and the polarization of the...
A mask quality control tool for the OSIRIS multi-object spectrograph
OSIRIS multi object spectrograph uses a set of user-customised-masks, which are manufactured on-demand. The manufacturing process consists of drilling the...
A Massive AGB Star as Source of Short-Lived Nuclei in the Early Solar System
The origin of short-lived radioactive nuclei at the time of the formation of the Sun is a much debated mystery in modern astronomy. We show that abundance...
A massive star odyssey : from main sequence to supernova : proceedings of the 212th Symposium of the International Astronomical Union held in Costa Teguise, Lanzarote, Canary Islands, 24-28 June 2002
A Method for Calibrating, in Absolute Flux Units, CA II H Profiles of Late Type Stars Observed at ESO
The authors have applied to the Sun a method for calibrating, in absolute flux units, Ca II H profiles of late-type stars. After comparing, in the region 3948 -...