activity
19952026
most citedThe European Large Area ISO Survey I: Goals, Definition and Observation

221 citations · 2.8k across the 68 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

15 papers · 1 filter

astro-ph.GA2026

Molecular Clouds Resolved at the Onset of Cosmic Noon

Bjorn Emonts, Matthew Lehnert, Mingyu Li +10

We present the discovery of seven molecular clouds in the radio galaxy B2 0902+34 at redshift z=3.4. These clouds are detected as CO(0-1) absorption features against the bright rad…

astro-ph.GA2024★ 10 cited

AGN feedback can produce metal enrichment on galaxy scales

Montse Villar-Martin, Carlos López Cobá, Sara Cazzoli +2

Giant (>100 kpc) nebulae associated with active galaxies provide rich information about the circumgalactic medium (CGM) around galaxies, its link with the interstellar medium (ISM)…

astro-ph.GA2024

Absorption of Millimeter-band CO and CN in the Early Universe: Molecular Clouds in Radio Galaxy B2 0902+34 at Redshift 3.4

Bjorn Emonts, Steve Curran, George Miley +9

Using the Karl G. Jansky Very Large Array (VLA), we have detected absorption lines due to carbon-monoxide, CO(J=0-1), and the cyano radical, CN(N=0-1), associated with radio galaxy…

astro-ph.GA2023★ 8 cited

CO survey of high-z radio galaxies, revisited with ALMA: Jet-cloud Alignments and Synchrotron Brightening by Molecular Gas in the Circumgalactic Environment

Bjorn Emonts, Matthew Lehnert, Sophie Lebowitz +6

Powerful radio sources associated with super-massive black holes are among the most luminous objects in the Universe, and are frequently recognized both as cosmological probes and…

astro-ph.GA2023★ 7 cited

The Dragonfly Galaxy. III. Jet-brightening of a High-redshift Radio Source Caught in a Violent Merger of Disk Galaxies

Sophie Lebowitz, Bjorn Emonts, Donald M. Terndrup +8

The Dragonfly Galaxy (MRC 0152-209), the most infrared-luminous radio galaxy at redshift z~2, is a merger system containing a powerful radio source and large displacements of gas.…

astro-ph.GA2023★ 29 cited

A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8

Bjorn H. C. Emonts, Matthew D. Lehnert, Ilsang Yoon +7

The growth of galaxies in the early Universe is driven by accretion of circum- and inter-galactic gas. Simulations predict that steady streams of cold gas penetrate the dark matter…

astro-ph.GA2021

Massive molecular outflow and 100 kpc extended cold halo gas in the enormous Ly nebula of QSO 1228+3128

Jianrui Li, Bjorn H. C. Emonts, Zheng Cai +9

The link between the circum-galactic medium (CGM) and the stellar growth of massive galaxies at high- depends on the properties of the widespread cold molecular gas. As part of…

astro-ph.GA2021★ 21 cited

Interactions between the large-scale radio structures and the gas in a sample of optically selected type 2 quasars

Montserrat Villar-Martin, Bjorn Emonts, Antonio Cabrera Lavers +5

The role of radio mode feedback in non radio-loud quasars needs to be explored in depth to determine its true importance. Its effects can be identified based on the evidence of int…

astro-ph.GA2019★ 16 cited

MUSE unravels the ionisation and origin of metal enriched absorbers in the gas halo of a z = 2.92 radio galaxy

S. Kolwa, J. Vernet, C. De Breuck +9

We have used the Multi-Unit Spectroscopic Explorer (MUSE) to study the circumgalactic medium (CGM) of a z = 2.92 radio galaxy, MRC 0943-242 by parametrising its emitting and absorb…

astro-ph.GA2018★ 74 cited

Giant galaxy growing from recycled gas: ALMA maps the circumgalactic molecular medium of the Spiderweb in [CI]

B. H. C. Emonts, M. D. Lehnert, H. Dannerbauer +9

The circumgalactic medium (CGM) of the massive Spiderweb Galaxy, a conglomerate of merging proto-cluster galaxies at z=2.2, forms an enriched interface where feedback and recycling…

astro-ph.GA2017★ 31 cited

Are we seeing accretion flows in a 250kpc-sized Ly-alpha halo at z=3?

J. Vernet, M. D. Lehnert, C. De Breuck +8

Using MUSE on the ESO-VLT, we obtained a 4 hour exposure of the z=3.12 radio galaxy MRC0316-257. We detect features down to ~10^-19 erg/s/cm^2/arcsec^2 with the highest surface bri…

astro-ph.GA2016★ 104 cited

Molecular Gas in the Halo Fuels the Growth of a Massive Cluster Galaxy at High Redshift

B. H. C. Emonts, M. D. Lehnert, M. Villar-Martin +19

The largest galaxies in the Universe reside in galaxy clusters. Using sensitive observations of carbon-monoxide, we show that the Spiderweb Galaxy -a massive galaxy in a distant pr…

astro-ph.GA2016★ 73 cited

Ionized outflows in luminous type 2 AGNs at z<0.6: no evidence for significant impact on the host galaxies

Montse Villar-Martin, Santiago Arribas, Bjorn Emonts +5

We investigate the presence of extended ionized outflows in 18 luminous type 2 AGNs (11 quasars and 7 high luminosity Seyfert 2s) at 0.3<z<0.6 based on VLT-FORS2 spectroscopy. We i…

astro-ph.GA2015★ 28 cited

A CO-rich merger shaping a powerful and hyper-luminous infrared radio galaxy at z=2: the Dragonfly Galaxy

B. H. C. Emonts, M. Y. Mao, A. Stroe +17

In the low-redshift Universe, the most powerful radio sources are often associated with gas-rich galaxy mergers or interactions. We here present evidence for an advanced, gas-rich…

astro-ph.GA2013★ 77 cited

CO(1-0) survey of high-z radio galaxies: alignment of molecular halo gas with distant radio sources

B. H. C. Emonts, R. P. Norris, I. Feain +19

We present a CO(1-0) survey for cold molecular gas in a representative sample of 13 high-z radio galaxies (HzRGs) at 1.4<z<2.8, using the Australia Telescope Compact Array. We dete…