The creation of carbon and oxygen in our Universe is one of the forefront questions in
nuclear astrophysics. The determination of the abundance of these elements is key to our …

Aims. We present the first public release of high-quality data products (DR1) from Hi-GAL,
the Herschel infrared Galactic Plane Survey. Hi-GAL is the keystone of a suite of continuum …

We present the first results from the science demonstration phase for the Hi-GAL survey, the
Herschel key program that will map the inner Galactic plane of the Milky Way in 5 bands. We …

Aims. For many years feedback processes generated by OB-stars in molecular clouds,
including expanding ionization fronts, stellar winds, or UV-radiation, have been proposed to …

We present a new catalogue of 5106 infrared bubbles created through visual classification
via the online citizen science website '; The Milky Way Project'. Bubbles in the new …

We describe the motivation, design, and implementation of the CORNISH survey, an
arcsecond-resolution radio continuum survey of the inner galactic plane at 5 GHz using the …

Several models have predicted that stars could form inside galactic outflows and that this
would be a new major mode of galaxy evolution. Observations of galactic outflows have …

We explore the variation in single-star 15–30${M} _ {\odot} $, nonrotating, solar metallicity,
pre-supernova MESA models that is due to changes in the number of isotopes in a fully …

FEEDBACK is a SOFIA (Stratospheric Observatory for Infrared Astronomy) legacy program
dedicated to study the interaction of massive stars with their environment. It performs a …

We unveil the stellar wind–driven shell of the luminous massive star-forming region of RCW
49 using SOFIA FEEDBACK observations of the [C ii] 158 μm line. The complementary data …