Neutral versus ionized gas kinematics at z ≃ 2.6: the AGN-host starburst galaxy PKS 0529-549

Author:

Lelli Federico1ORCID,De Breuck Carlos1,Falkendal Theresa12,Fraternali Filippo3,Man Allison W S1,Nesvadba Nicole P H4,Lehnert Matthew D2

Affiliation:

1. European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching bei München, Germany

2. Sorbonne Université, CNRS UMR 7095, Institut d’Astrophysique de Paris, 98 bis bd Arago, F-75014 Paris, France

3. Kapteyn Astronomical Institute, University of Groningen, Postbus 800, NL-9700 AV, Groningen, the Netherlands

4. Institut d’Astrophysique Spatiale, UMR 8617, Université Paris-Sud, Bât. 121, F-91405, Orsay, France

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. JWST Reveals a Surprisingly High Fraction of Galaxies Being Spiral-like at 0.5 ≤ z ≤ 4;The Astrophysical Journal Letters;2024-06-01

2. KAOSS: turbulent, but disc-like kinematics in dust-obscured star-forming galaxies at z ∼ 1.3–2.6;Monthly Notices of the Royal Astronomical Society;2024-04-23

3. Galaxy kinematics and mass estimates at z ∼ 1 from ionized gas and stars;Monthly Notices of the Royal Astronomical Society;2023-11-27

4. The ALMA-ALPAKA survey;Astronomy & Astrophysics;2023-11

5. B/PS bulges and barlenses from a kinematic viewpoint – I;Monthly Notices of the Royal Astronomical Society;2023-09-05

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