Sensitive Herschel far-infrared observations can break degeneracies that were inherent to previous studies of star formation in high-z AGN hosts. Combining PACS...

It has been well established in the past decades that the central black hole masses of galaxies correlate with dynamical properties of their harbouring bulges...

The star formation main sequence (SFMS) is a tight relation between the galaxy star formation rate (SFR) and its total stellar mass (M⋆). Early-type galaxies...

Large-scale propagating star formation in galaxies is studied as a self-regulatin process. The model connects the energy injection by star formation with the...

Aims: We investigate the star formation history of the IC1396 region by studying its kinematics and completing the population census. Methods: We used...

We present a study of the star formation in the giant Hii region NGC5471 in the outskirts of M101. We have performed integrated photometry of the mean emission...

An objective prism H alpha survey has shown that there is a population of early type spiral galaxies in nearby clusters with strong central bursts of star...

Aims: Though S0 galaxies are usually thought to be `red and dead', they often demonstrate weak star formation organised in ring structures and located in their...

We present narrowband observations of the Hα emission in a sample of 31 satellites orbiting isolated giant spiral galaxies. The sample studied spans the range...