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Massive molecular gas reservoir around the central AGN in the CARLA J1103+3449 cluster at z=1.44
- Source :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 641, pp.A22. ⟨10.1051/0004-6361/202038673⟩
- Publication Year :
- 2020
- Publisher :
- arXiv, 2020.
-
Abstract
- Passive early-type galaxies dominate cluster cores at z $\lesssim$1.5. At higher redshift, cluster core galaxies are observed to have still on-going star-formation, fuelled by cold molecular gas. We measure the molecular gas reservoir of the central region around the radio-loud AGN in the cluster CARLA J1103+3449 at z=1.44 with NOEMA. The AGN synchrotron emission dominates the continuum emission at 94.48 GHz, and we measure its flux at the AGN position and at the position of two radio jets. Combining our measurements with published results over the range 4.71 GHz-94.5 GHz, we obtain a flat spectral index $\alpha = 0.14 \pm 0.03$ for the AGN core emission, and a steeper index $\alpha = 1.43 \pm 0.04$ and $\alpha = 1.15 \pm 0.04$ at positions close to the western and eastern lobe, respectively. The total spectral index is $\alpha = 0.92 \pm 0.02$ over the range 73.8 MHz-94.5 GHz. We detect two CO(2-1) emission lines, both blue-shifted with respect to the AGN. Their emission corresponds to two regions, ~17 kpc south-east and ~14 kpc south-west of the AGN, not associated with galaxies. In these two regions, we find a total massive molecular gas reservoir of $M_{gas}$ = 3.9 $\pm$ 0.4 $10^{10} M_{\odot}$, which dominates (~ 60%) the central total molecular gas reservoir. These results can be explained by massive cool gas flows in the center of the cluster. The AGN early-type host is not yet quenched; its star formation rate is consistent with being on the main sequence of star-forming galaxies in the field (SFR~30-140 $M_{\odot}$/yr), and the cluster core molecular gas reservoir is expected to feed the AGN and the host star-formation before quiescence. The other cluster confirmed members show star formation rates at ~2 $\sigma$ below the field main sequence at similar redshifts and do not have molecular gas masses larger than galaxies of similar stellar mass in the field.<br />Comment: 18 pages, 14 figures, A&A, accepted for publication
- Subjects :
- Active galactic nucleus
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Stellar mass
Astrophysics::High Energy Astrophysical Phenomena
FOS: Physical sciences
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
galaxies: clusters: individual: CARLA J1103 + 3449
0103 physical sciences
Emission spectrum
010303 astronomy & astrophysics
Astrophysics::Galaxy Astrophysics
Physics
radio continuum: galaxies
Spectral index
010308 nuclear & particles physics
Star formation
Astronomy and Astrophysics
galaxies: jets
Astrophysics - Astrophysics of Galaxies
Galaxy
Redshift
Synchrotron emission
13. Climate action
Space and Planetary Science
galaxies: star formation
Astrophysics of Galaxies (astro-ph.GA)
Astrophysics::Earth and Planetary Astrophysics
galaxies: evolution
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Astrophysics - Cosmology and Nongalactic Astrophysics
Subjects
Details
- ISSN :
- 00046361
- Database :
- OpenAIRE
- Journal :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 641, pp.A22. ⟨10.1051/0004-6361/202038673⟩
- Accession number :
- edsair.doi.dedup.....5cef4ebe9ea1ccdbd263df120b42ceac
- Full Text :
- https://doi.org/10.48550/arxiv.2007.03706