activity
20142026
most citedKinematics and physical conditions of HI in nearby radio sources. The last survey of the old Westerbork Synthesis Radio Telescope

86 citations · 930 across the 63 of their papers we have counts for

collaborators

65 papers

astro-ph.GA2026

A search for HI absorption in distant star-forming galaxies with ASKAP-FLASH - II. Direct observations and stacking of 21 cm line

Sophie L. Eden, Elaine M. Sadler, Kevin A. Pimbblet +5

We present results of a search for associated and intervening HI 21 cm absorption in star-forming galaxies and a control sample of radio galaxies at 0.4 < < 1.0, using ASKAP's…

astro-ph.GA2026

From Atomic Gas to Star Formation

Erik Rosolowsky, Eric Koch, Sambit Roychowdhury +9

Since the 2015 SKA Chapters, the advent of panchromatic observations of nearby galaxies, capable of resolving the interstellar medium (ISM) into individual star-forming regions and…

astro-ph.GA2026

The Bright Future of the Dark and Dim Universe

N. Deg, Alejandro Benitez-Llambay, Elizabeth A. K. Adams +5

This chapter investigates the low-mass frontier of galaxy formation through two complementary populations: the starless Reionization-Limited HI Clouds (RELHICs) that trace the ``da…

astro-ph.GA2026

AGN Feeding & Feedback Over the Galactic Scales

Filippo M. Maccagni, Vincenzo Mainieri, Isabella Prandoni +8

Active Galactic Nuclei (AGN) are key drivers of galaxy evolution, triggered by cold gas accreting onto a super-massive black hole. However, the processes regulating this gas accret…

astro-ph.GA2026

Tracing Cold Gas in Absorption Across Cosmic Time with the SKA

Elizabeth K. Mahony, Neeraj Gupta, Sergei A. Balashev +12

Observing the 21-cm HI line in absorption provides a powerful means of tracing the cold neutral gas in normal and active galaxies across cosmic time. The frequency coverage and sen…

astro-ph.GA2026

Insights into Jet-Induced Cloud Disruption in NGC 1316: ALMA Reveals a Spatially Extended Molecular Gas

Kana Morokuma-Matsui, Alexander Y. Wagner, Filippo M. Maccagni +14

We present ALMA CO() observations of a nearby radio galaxy NGC1316 at a 100-pc resolution to investigate the impact of AGN jets on the molecular gas. The molecular gas exhib…

astro-ph.GA2026

Deep HI observations of cold gas inflow and outflow

W. J. G. de Blok, D. B. Fisher, K. Tachihara +8

A major question in galaxy evolution is how galaxies acquire sufficient gas to sustain their star formation rates. HI observations with high angular resolution and sensitivity to v…

astro-ph.CO2026

The Impact of Dense RM Grids on the Study of Intra-cluster and Intra-group Magnetic Fields

Francesca Loi, Valentina Vacca, Shane P. O'Sullivan +8

The presence of diffuse radio sources in galaxy clusters and the recent discovery of polarized signals associated with the tails of a jellyfish galaxy indicates that intra-cluster/…

astro-ph.GA2026

The ultra-deep HI radial profiles of late-type galaxies from MHONGOOSE

S. Veronese, W. J. G. de Blok, E. Brinks +4

Galaxy discs have a finite extent, yet how and where their neutral atomic hydrogen (HI) components end is not fully understood. The existence of a break in the HI disc at column de…

astro-ph.HE2026

BlackHoleWeather -- Jet-regulated chaotic cold accretion across the meso scale: Variability and kinematics

Vieri Cammelli, Massimo Gaspari, Filippo Barbani +10

Chaotic cold accretion (CCA) predicts that supermassive black holes are fed by multiphase clouds condensing from turbulent hot atmospheres. In jet-regulated systems cold gas must a…

astro-ph.GA2026

BlackHoleWeather -- Spin-coupled chaotic cold accretion across the meso scale: Variability and kinematics

Olmo Piana, Massimo Gaspari, Vieri Cammelli +10

Supermassive black hole (SMBH) spin records the vector history of accretion. In chaotic cold accretion (CCA), this history is set by clouds and filaments whose torques can add cohe…

astro-ph.GA2026

BlackHoleWeather -- Chaotic cold accretion across the meso-scale: Morphology and thermodynamics

Filippo Barbani, Massimo Gaspari, Vieri Cammelli +12

Supermassive black holes (SMBHs) self-regulate galaxies, groups, and clusters, yet the pathway transporting gas from halo scales to sub-pc radii remains debated. In hot stratified…

astro-ph.GA2026

BlackHoleWeather -- Chaotic cold accretion across the meso-scale: Variability and kinematics

Filippo Barbani, Massimo Gaspari, Olmo Piana +12

Accretion onto supermassive black holes (SMBHs) in realistic halos is time-variable, governed by turbulence, cooling, and multiphase condensation. In chaotic cold accretion (CCA),…

astro-ph.GA2026

BlackHoleWeather -- Jet-regulated chaotic cold accretion across the meso scale: Morphology and thermodynamics

Vieri Cammelli, Massimo Gaspari, Olmo Piana +11

How mechanical AGN feedback couples to multiphase condensation across scales remains a problem in galaxy groups and clusters. It is unclear how jets reshape the chaotic cold accret…

astro-ph.GA2026

BlackHoleWeather -- Spin-coupled chaotic cold accretion across the meso-scale: Morphology and thermodynamics

Olmo Piana, Massimo Gaspari, Filippo Barbani +10

Supermassive black hole (SMBH) spin is a key but poorly constrained ingredient of the feeding-feedback loop. Chaotic cold accretion (CCA) of cold gas clouds delivers rapidly varyin…

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.CO2026

The MeerKAT Fornax Survey VII. Characterisation of the Fornax cluster's magnetic field and new insights on magnetisation in large scale systems

Francesca Loi, Matteo Murgia, Federica Govoni +5

Large scale magnetic fields in galaxy clusters can influence their physics and the evolution of the cluster galaxies. These properties remain poorly constrained due to a historical…

astro-ph.GA2026

FEASTS and MHONGOOSE: HI Column Density Distribution at for

Jing Wang, Xuchen Lin, Ze-Zhong Liang +24

We present the first HI column density distribution function, , extending down to . This was derived from high-s…

astro-ph.GA2025

Baryonic Masses and Properties of Gaseous Satellite Galaxies

Jingyao Zhu, Yasmeen Asali, Mary Putman +12

We present a sample of 127 gas-bearing dwarf galaxies around 56 late-type host galaxies within 30 Mpc using 21-cm HI data from the WALLABY, MHONGOOSE, and ALFALFA surveys. We chara…

astro-ph.GA2025

The inside-out quenching of the MHONGOOSE galaxy NGC 1371

S. Veronese, W. J. G. de Blok, F. Fraternali +5

We present the deepest 21-cm spectral line and 1.4 GHz broad-band continuum observations of nearby early-type spiral galaxy NGC 1371 as part of the MeerKAT HI Observations of Nearb…

astro-ph.GA2025

HI gas in the rejuvenated radio galaxy PKS 2014-55

Leon Mtshweni, Kshitij Thorat, Roger P. Deane +17

We present new high-spectral-resolution MeerKAT observations of absorption against the central region of the restarted, giant, X-shaped radio galaxy PKS2014-55, which…

astro-ph.GA2025

The MeerKAT Fornax Survey: removal of HI gas from galaxies in the Fornax cluster

F. M. Maccagni, P. Serra

The MeerKAT Fornax Survey is conducting a thorough examinationof the nearby Fornax galaxy cluster to understand how galaxies lose their cold gas and stop forming stars in low-mass…

astro-ph.GA2025

Atomic hydrogen reservoirs in quiescent galaxies at z = 0.4

A. Bianchetti, G. Rodighiero, D. Donevski +11

Context. Based on Local Universe observations, quiescent galaxies (QGs) host lower to no HI compared to star-forming galaxies (SFGs), but no constraints have been derived so far at…

astro-ph.GA2025

MeerKAT Discovery of an Infalling Cold Gas Tail onto the Nearby Barred Spiral Galaxy, NGC 5643

K. C. Santana, F. M. Maccagni, R. Deane +1

The detailed study of gas flows in local Active Galactic Nuclei (AGN) is essential for understanding the regulation of star formation and black hole growth, which are fundamental t…