We present azimuthally-averaged spectral energy distributions (SEDs) from FUV to FIR, as a function of radius, for the galaxies included in the SINGS sample...

Preliminary results from spatially resolved spectroscopy and photometry of the star-forming dwarf galaxy II Zw 33 are presented. Our study has revealed the...

The relation known as Star Formation Main Sequence (SFMS) of galaxies is defined in terms of stellar mass and star formation rate. This approximately linear...

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The dwarf elliptical galaxies (dEs) are more luminous than dwarf spheroidals and fainter than "normal" ellipticals. In this paper I investigate the...

Near-infrared interferometry gives us the opportunity to spatially resolve the circumstellar environment of young stars at sub-astronomical-unit (au) scales...

The angular resolution of the Very Large Telescope Interferometer (VLTI) and the excellent sensitivity of GRAVITY have led to the first detection of spatially...

Galaxies in voids have been found to be of a later type, bluer, less massive, and to have a slower evolution than galaxies in denser environments (filaments and...