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 …

Nearby galaxies offer unique laboratories allowing multi-wavelength spatially resolved
studies of the interstellar medium, star formation and nuclear activity across a broad range of …

Using spectral line observations of HNCO, N2H+, and HNC, we investigate the kinematics of
dense gas in the central∼ 250 pc of the Galaxy. We present scouse (Semi-automated multi …

ABSTRACT The Plateau de Bure Interferometer Arcsecond Whirlpool Survey has mapped
the molecular gas in the central∼ 9 kpc of M51 in its 12 CO (1–0) line emission at a cloud …

Ethanol (CH3CH2OH) is a relatively common molecule, often found in star-forming regions.
Recent studies suggest that it could be a parent molecule of several so-called interstellar …

We present the first unbiased molecular line survey toward an extragalactic source, namely
the nuclear region of the starburst galaxy NGC 253. The scan covers the frequency band …

Aims. We present a detailed analysis of Atacama Large Millimeter/submillimeter Array
(ALMA) Bands 7 and 9 data of CO, HCO+, HCN, and CS, augmented with Plateau de Bure …

We present spatially resolved (∼ 50 pc) imaging of molecular gas species in the central
kiloparsec of the nearby starburst galaxy NGC 253, based on observations taken with the …

The current generation of (sub) mm-telescopes has allowed molecular line emission to
become a major tool for studying the physical, kinematic, and chemical properties of …

We present hydrodynamic simulations of the interstellar medium (ISM) within the
circumnuclear disc (CND) of a typical active galactic nucleus (AGN)-dominated galaxy …