activity
20242026
most citedOutflowing shocked gas dominates the NIR H emission from the dual AGN NGC6240

3 citations · 3 across the 4 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

20 papers · 1 filter

astro-ph.GA2026

Spatially resolved molecular gas conditions in the circumnuclear disc of 3C 84

Bin Jia, Tom Oosterloo, Serena Viti +1

The brightest cluster galaxy NGC 1275, at the centre of the Perseus cluster, hosts the radio-loud AGN 3C 84 and a circumnuclear disc (CND) of cold molecular gas onto which large-sc…

astro-ph.GA2026

HI Galaxy Science with the SKA

Jing Wang, D. J. Pisano, Sarah Blyth +9

This chapter introduces the contributions of the HI galaxy science in this volume reviewing the latest developments and urgent questions in HI galaxy science, providing guiding pri…

astro-ph.GA2026

HI absorption in MHONGOOSE -- Spin temperatures and cold neutral medium in nearby disk galaxies

W. J. G. de Blok, F. M. Maccagni, L. Chemin +7

Combined HI emission-absorption studies constrain the spin temperature and phase structure of the neutral atomic hydrogen interstellar medium (ISM), but have largely been limited t…

astro-ph.GA20263 cited

Outflowing shocked gas dominates the NIR H emission from the dual AGN NGC6240

J. Carlsen, C. Cicone, B. Hagedorn +10

[Abridged] We present a multi-line study of the kinematics of the molecular and ionised gas phases in the central 2 kpc of NGC6240, based on JWST/NIRSpec and ALMA observations. We…

astro-ph.GA2026

A deep MeerKAT view of associated HI absorption in radio AGNs at intermediate redshift: Role of absorber geometry and conditions of the gas

Raffaella Morganti, Tom Oosterloo, Clive Tadhunter +1

We present MeerKAT observations searching for HI absorption in a sample of 17 powerful ( W Hz) radio sources at intermediate redshifts (

astro-ph.GA2026

Not so-dark: High resolution HI imaging of J0139+4328 and identification of an optical counterpart

Barbara Å iljeg, Elizabeth A. K. Adams, Tom A. Oosterloo +4

Dark galaxies - systems rich in neutral hydrogen (HI) gas but with no stars - are a common prediction of numerous theoretical models and cosmological simulations. However, the uneq…