activity
19932025
most citedHow to Calculate Molecular Column Density

418 citations · 1.8k across the 45 of their papers we have counts for

collaborators

45 papers

astro-ph.IM2025

Environmental Monitoring Requirements for the ngVLA

T. K. Sridharan, J. G. Mangum, B. Butler

Measurement of environmental parameters is one of the basic requirements for the proper operation of a telescope. This memo is intended to provide guidance for the measurement accu…

astro-ph.HE2025★ 8 cited

Millimeter emission from supermassive black hole coronae

S. del Palacio, C. Yang, S. Aalto +28

Active Galactic Nuclei (AGN) host accreting supermassive black holes (SMBHs). The accretion can lead to the formation of a hot, X-ray emitting corona close to the SMBH capable of a…

astro-ph.GA2025★ 4 cited

Shock-induced HCNH+ abundance enhancement in the heart of the starburst galaxy NGC 253 unveiled by ALCHEMI

Y. Gong, C. Henkel, C. T. Bop +15

Understanding the chemistry of molecular clouds is pivotal to elucidate star formation and galaxy evolution. As one of the important molecular ions, HCNH+ plays an important role i…

astro-ph.GA2024★ 8 cited

An ALCHEMI inspection of sulphur-bearing species towards the central molecular zone of NGC 253

M. Bouvier, S. Viti, E. Behrens +19

Sulphur-bearing species are detected in various environments within Galactic star-forming regions and are particularly abundant in the gas phase of outflows and shocks, and photo-d…

astro-ph.GA2024

Physical Properties of the Southwest Outflow Streamer in the Starburst Galaxy NGC 253 with ALCHEMI

Min Bao, Nanase Harada, Kotaro Kohno +19

The physical properties of galactic molecular outflows are important as they could constrain outflow formation mechanisms. We study the properties of the southwest (SW) outflow str…

astro-ph.GA2024★ 5 cited

A spectacular galactic scale magnetohydrodynamic powered wind in ESO 320-G030

M. D. Gorski, S. Aalto, S. König +23

How galaxies regulate nuclear growth through gas accretion by supermassive black holes (SMBHs) is one of the most fundamental questions in galaxy evolution. One potential way to re…