output
19922026
most citedMeasurements of Omega and Lambda from 42 High-Redshift Supernovae

18.1k citations

Showing 2022 · astro-ph.GAShow all

34 papers · 2 filters

astro-ph.GA2022★ 16 cited

Radio jet-ISM interaction and positive radio-mechanical feedback in Abell 1795

Prathamesh D. Tamhane, Brian R. McNamara, Helen R. Russell +8

We present XSHOOTER observations with previous ALMA, MUSE and observations to study the nature of radio-jet triggered star formation and the interaction of radio jets with th…

astro-ph.GA2022★ 15 cited

The origin of double-peak emission-line galaxies: rotating discs, bars or galaxy mergers?

Daniel Maschmann, Anaelle Halle, Anne-Laure Melchior +2

Emission lines with a double-peak (DP) shape, detected in the centre of galaxies, have been extensively used in the past to identify peculiar kinematics such as dual active galacti…

astro-ph.GA2022★ 13 cited

Tracing the kinematics of the whole ram pressure stripped tails in ESO 137-001

Rongxin Luo, Ming Sun, Pavel Jáchym +8

Ram pressure stripping (RPS) is an important process to affect the evolution of cluster galaxies and their surrounding environment. We present a large MUSE mosaic for ESO 137-001 a…

astro-ph.GA2022

Origin of the differences in rotational support among early-type galaxies: The case of galaxies outside clusters

Michal Bílek, Pierre-Alain Duc, Elisabeth Sola

Context: Early-type galaxies (ETGs) are divided into slow and fast rotators (FRs and SRs) according to the degree of ordered rotation of their stellar populations. Cosmological hyd…

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…