As part of an extensive study of the physical properties of active galactic nuclei (AGNs) we
report high spatial resolution near-IR integral-field spectroscopy of the narrow-line region …

We present an updated mid-infrared (MIR) versus X-ray correlation for the local active
galactic nuclei (AGN) population based on the high angular resolution 12 and 18μm …

We use ALMA observations to derive mass, length, and time scales associated with NGC
253's nuclear starburst. This region forms∼ 2 M☉ yr− 1 of stars and resembles other …

We present the first subarcsecond-resolution mid-infrared (MIR) atlas of local active galactic
nuclei (AGN). Our atlas contains 253 AGN with a median redshift of z= 0.016, and includes …

We analyze HCN and HNC emission in the nearby starburst galaxy NGC 253 to investigate
its effectiveness in tracing heating processes associated with star formation. This study uses …

We present a detailed study of a molecular outflow feature in the nearby starburst galaxy
NGC 253 using ALMA. We find that this feature is clearly associated with the edge of NGC …

Context. The interstellar medium is the locus of physical processes affecting the evolution of
galaxies which drive or are the result of star formation activity, supermassive black hole …

We analyze image and spectral data from≈ 365 ks of observations from the Chandra X-ray
Observatory of the nearby, edge-on starburst galaxy NGC 253 to constrain properties of the …

The center of the nearby galaxy NGC 253 hosts a population of more than a dozen super
star clusters (SSCs) that are still in the process of forming. The majority of the star formation …

Abstract We present 0 farcs 15 (∼ 2.5 pc) resolution ALMA CO (3–2) observations of the
starbursting center in NGC 253. Together with archival ALMA CO (1–0) and CO (2–1) data …