ELMER is a multi-purpose instrument for the GTC designed for both, imaging and spectroscopy in the visible range. The detection subsystem consists of a single...
R stars are carbon stars, less luminous and hotter than the carbon stars evolving along the AGB phase. Thus, their carbon enrichment cannot be a consequence of...
The embedded cluster IRAS17136 - 3617 associated with the nebulosity GM24
Radio, infrared, and optical observations of the embedded infrared cluster IRAS17136 - 3617 are reviewed. The cluster consists of more than 25 stars with a...
The Emergence of Magnetic Field into Stellar Atmospheres
The magnetic activity in the atmosphere of the Sun, possibly of most other magnetically active late-type stars, is a consequence of the emergence of magnetic...
The EMIR experience in the use of software control simulators to speed up the time to telescope
One of the main problems facing development teams working on instrument control systems consists on the need to access mechanisms which are not available until...
The EMIR Near-Infrared Multi-Object Spectrograph for GTC
EMIR is a near-infrared (NIR) multi-object spectrograph (MOS) proposed for first-generation common user instrument of the Gran Telescopio Canarias GTC. It has...
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...