EMIR is a multiobject intermediate resolution near infrared (1.0 - 2.5 microns) spectrograph with image capabilities to be mounted on the Gran Telescopio...
There is increasing evidence that there is a major bar in the inner Galaxy. The distance to near end of the bar at l = 27° has been directly measured by using...
The emission line shapes of the Seyfert 1 galaxy Mrk 817
The analysis of emission line region of Seyfert 1 galaxy Mrk 817 is presented. We found that emission line region in Mrk 817 is very complex. Moreover, the...
The Energetic Particle Detector Suite for Solar Orbiter
Multiple processes in the solar atmosphere or near the Sun are capable of energizing electrons and ions which are remotely observed as Solar Energetic Particle...
The Engineering Behind Mars Exploration Program 2007 Phoenix Mission Landing Site Selection
This abstract details the engineering processes used in the overall landing site selection process. The performance of the landing RADAR, IMU, thrusters and...
The ENLR of NGC 4151 - Spatial variations of the line ratios
The first results of an analysis of the spatial variations along and across the ENLR of NGC 4151 are presented. The excitation of the gas clearly decreases with...
The entangled red giant branch area near the horizontal-branch in color-magnitude diagrams of nearby galaxies: discovery of the AGB-bump.
Recently, huge photometric databases are being obtained for the Magellanic Clouds and other Local Group galaxies. These data allow, not only to study in great...
Massive galaxies experienced an enormous structural evolution in the last ten billion years. The most viable explanation is that massive galaxies have undergone...