activity
20002023
most citedRelativistic Jets in Active Galactic Nuclei

845 citations · 4.3k across the 84 of their papers we have counts for

collaborators

85 papers

astro-ph.GA2023★ 1 cited

Widespread Hot Ammonia in the Central Kiloparsec of the Milky Way

Tierra M. Candelaria, E. A. C Mills, David S. Meier +2

The inner 300-500 pc of the Milky Way has some of the most extreme gas conditions in our Galaxy. Physical properties of the Central Molecular Zone (CMZ), including temperature, den…

astro-ph.GA2022★ 43 cited

Tracing Interstellar Heating: An ALCHEMI Measurement of the HCN Isomers in NGC 253

Erica Behrens, Jeffrey G. Mangum, Jonathan Holdship +17

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…

astro-ph.GA2022★ 18 cited

ALCHEMI finds a "shocking" carbon footprint in the starburst galaxy NGC~253

Nanase Harada, Sergio Martin, Jeff Mangum +15

Centers of starburst galaxies may be characterized by a specific gas and ice chemistry due to their gas dynamics and the presence of various ice desorption mechanisms. This may res…

astro-ph.GA2022★ 6 cited

Down but not out: properties of the molecular gas in the stripped Virgo Cluster early-type galaxy NGC4526

Lisa M. Young, David S. Meier, Alison Crocker +2

We present ALMA data on the 3mm continuum emission, CO isotopologues (12CO, 13CO, C18O), and high-density molecular tracers (HCN, HCO+, HNC, HNCO, CS, CN, and CH3OH) in NGC4526. Th…

astro-ph.GA2022★ 29 cited

Methanol masers in NGC 253 with ALCHEMI

P. K. Humire, C. Henkel, A. Hernández-Gómez +23

Context: Methanol masers of Class I (collisionally-pumped) and Class II (radiatively-pumped) have been studied in great detail in our Galaxy in a variety of astrophysical environme…

astro-ph.GA2022★ 27 cited

A 2-3 mm high-resolution molecular line survey towards the centre of the nearby spiral galaxy NGC 6946

Cosima Eibensteiner, Ashley T. Barnes, Frank Bigiel +30

The complex physical, kinematic, and chemical properties of galaxy centres make them interesting environments to examine with molecular line emission. We present new " (${\sim…