Observations that resolve nearby galaxies into individual regions across multiple phases of
the gas–star formation feedback “matter cycle” have provided a sharp new view of molecular …

We present the PHANGS-MUSE survey, a programme that uses the MUSE integral field
spectrograph at the ESO VLT to map 19 massive (9.4< log (M⋆/M⊙)< 11.0) nearby (D≲ 20 …

We utilize medium-resolution JWST/NIRSpec observations of 164 galaxies at z= 2.0–9.3
from the Cosmic Evolution Early Release Science (CEERS) survey to investigate the …

The processes of star formation and feedback, regulating the cycle of matter between gas
and stars on the scales of giant molecular clouds (GMCs;∼ 100 pc), play a major role in …

Ionized nebulae provide critical insights into the conditions of the interstellar medium (ISM).
Their bright emission lines enable the measurement of physical properties, such as the gas …

We measure empirical relationships between the local star formation rate (SFR) and
properties of the star-forming molecular gas on 1.5 kpc scales across 80 nearby galaxies …

The first JWST observations of nearby galaxies have unveiled a rich population of bubbles
that trace the stellar-feedback mechanisms responsible for their creation. Studying these …

Polycyclic aromatic hydrocarbons (PAHs) play a critical role in the reprocessing of stellar
radiation and balancing the heating and cooling processes in the interstellar medium but …

Large-scale bars can fuel galaxy centers with molecular gas, often leading to the
development of dense ringlike structures where intense star formation occurs, forming a very …

The nebular recombination line H α is widely used as a star formation rate (SFR) indicator in
the local and high-redshift Universe. We present a detailed H α radiative transfer study of …