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20012023
most citedA Galaxy-Scale Fountain of Cold Molecular Gas Pumped by a Black Hole

124 citations · 1k across the 55 of their papers we have counts for

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15 papers · 1 filter

astro-ph.GA2022★ 8 cited

The Close AGN Reference Survey (CARS). A parsec scale multi-phase outflow in the super-Eddington NLS1 Mrk 1044

Nico Winkel, Bernd Husemann, Mainak Singha +8

The interaction between Active Galactic Nuclei (AGN) and their host galaxies is scarcely resolved. Narrow-line Seyfert 1 (NLS1) galaxies are believed to represent AGN at early stag…

astro-ph.GA2022★ 16 cited

Does absorption against AGN reveal supermassive black hole accretion?

Tom Rose, B. R. McNamara, F. Combes +7

Galaxies often contain large reservoirs of molecular gas which shape their evolution. This can be through cooling of the gas -- which leads to star formation, or accretion onto the…

astro-ph.GA2022★ 44 cited

The distribution of globular clusters in kinematic spaces does not trace the accretion history of the host galaxy

Giulia Pagnini, Paola Di Matteo, Sergey Khoperskov +4

Reconstructing how all the stellar components of the Galaxy formed and assembled over time, by studying the properties of the stars which make it, is the aim of Galactic archeology…

astro-ph.GA2022★ 45 cited

Physics of ULIRGs with MUSE and ALMA: PUMA IV. No tight relation between cold molecular outflow rates and AGN luminosities

I. Lamperti, M. Pereira-Santaella, M. Perna +11

We study molecular outflows in a sample of 25 nearby (z< 0.17, d<750 Mpc) ULIRG systems (38 individual nuclei) as part of the "Physics of ULIRGs with MUSE and ALMA" (PUMA) survey,…

astro-ph.GA2022★ 9 cited

Mapping HI 21-cm in the Klemola 31 group at z = 0.029: emission and absorption towards PKS2020-370

E. K. Maina, Abhisek Mohapatra, G. I. G. Jozsa +11

We present MeerKAT Absorption Line Survey (MALS) observations of the HI gas in the Klemola31 galaxy group (), located along the line of sight to the radio-loud quasar PKS2…

astro-ph.GA2022★ 11 cited

Star forming and gas rich brightest cluster galaxies at in the Kilo-Degree Survey

G. Castignani, M. Radovich, F. Combes +9

Brightest Cluster Galaxies (BCGs) are typically massive ellipticals at the centers of clusters. They are believed to experience strong environmental processing, and their mass asse…

astro-ph.HE2022★ 61 cited

First discoveries and localisations of Fast Radio Bursts with MeerTRAP: a real-time, commensal MeerKAT survey

K. M. Rajwade, M. C. Bezuidenhout, M. Caleb +24

We report on the discovery and localization of fast radio bursts (FRBs) from the MeerTRAP project, a commensal fast radio transient-detection programme at MeerKAT in South Africa.…

astro-ph.GA2022★ 15 cited

The Close AGN Reference Survey (CARS): Tracing the circumnuclear star formation in the super-Eddington NLS1 Mrk 1044

N. Winkel, B. Husemann, T. A. Davis +11

The host galaxy conditions for rapid supermassive black hole growth are poorly understood. Narrow-line Seyfert 1 (NLS1) galaxies often exhibit high accretion rates and are hypothes…

astro-ph.GA2022

Linking pressure gradients with the stability of molecular clouds in galactic outflows

K. M. Dasyra, G. F. Paraschos, T. Bisbas +2

The jets launched by actively accreting black holes are capable of launching several of the massive (million or billion solar mass) molecular outflows observed in galaxies. These o…

astro-ph.GA2022★ 11 cited

NOEMA observations support a recoiling black hole in 3C186

G. Castignani, E. Meyer, M. Chiaberge +7

3C186 is a powerful radio loud quasar (QSO) at the center of a cool-core cluster at z=1.06. Previous studies reported evidence for a projected spatial offset of ~1'' between the is…

astro-ph.GA2022★ 13 cited

CO in the ALMA Radio-Source Catalogue (ARC): the molecular gas content of radio galaxies as a function of redshift

A. Audibert, K. M. Dasyra, M. Papachristou +6

To evaluate the role of radio activity in galaxy evolution, we designed a large archival CO survey of radio galaxies (RGs) to determine their molecular gas masses at different epoc…

astro-ph.GA2022★ 6 cited

HI gas playing hide-and-seek around a powerful FRI-type quasar at z2.1

N. Gupta, R. Srianand, E. Momjian +5

We present optical spectroscopic and milli-arcsecond scale radio continuum observations of the quasar M1540-1453 ( = 2.1040.002) that shows associated HI 21-cm absorpt…

astro-ph.GA2022★ 3 cited

Unveiling the Main Sequence to Starburst Transition Region with a Sample of Intermediate Redshift Luminous Infrared Galaxies

L. Hogan, D. Rigopoulou, S. García-Burillo +8

We present a CO(3-2) study of four systems composed of six (ultra) luminous infrared galaxies (U/LIRGs), located at 0.28 < z < 0.44, that straddle the transition region between reg…

astro-ph.GA2022★ 5 cited

Non-star-forming molecular gas in the Abell 1367 intra-cluster multiphase orphan cloud

Pavel Jáchym, Ming Sun, Masafumi Yagi +7

We report the detection of CO emission in the recently discovered multiphase isolated gas cloud in the nearby galaxy cluster Abell 1367. The cloud is located about 800 kpc in proje…

astro-ph.GA2022★ 40 cited

Gas condensation in Brightest Group Galaxies unveiled with MUSE

V. Olivares, P. Salome, S. L. Hamer +18

The origin of the cold gas in central galaxies in groups is still a matter of debate. We present Multi-Unit Spectroscopic Explorer (MUSE) observations of 18 optically selected loca…