High contrast and high resolution optical imaging from the ground: results from FASTCAM at NOT and WHT
Developed since 2006 by the IAC and UPCT, FASTCAM is an optical camera which takes advantage of recently available low noise and fast read-out CCDs (with...
High-resolution optical spectroscopy for everyone: want a PEPSI?
The demand of high-res spectroscopy had seen a tremendous increase after the discovery of exoplanets. Such instruments are now among the standard equipment of...
HORuS: High-Resolution and Broad Spectral Coverage on GTC
The High Optical Resolution Spectrograph (HORuS), is now ready for operation on Gran Telescopio Canarias (GTC). HORuS is mainly a recyled instrument, largely...
Hot Bubbles in Nebulae around Evolved Stars: probing stellar evolution
In this talk we will present our most recent numerical and observational results on the formation, evolution, and X-ray emission from hot bubbles in nebulae...
How does the group environment hamper star-formation in star-forming galaxies?
How does the group environment hamper star-formation in star-forming galaxies? Abstract: We present the first results from the H-alpha Galaxy Groups Imaging...
How dynamical environment regulates the structure of the molecular gas and star formation in M51
Gas kinematics on the scales of Giant Molecular Clouds (GMCs) are essential for probing the framework that links the large-scale organization of interstellar...
How dynamical environment regulates the structure of the molecular gas and star formation in M51
Gas kinematics on the scales of Giant Molecular Clouds (GMCs) are essential for probing the framework that links the large-scale organization of interstellar...
How massive galaxies have evolved over cosmic time?
In the last few years there has been cumulative evidence showing that massive galaxies have dramatically grown in size since z~3. This result has remained very...