The quasar feedback survey: discovering hidden Radio-AGN and their connection to the host galaxy ionized gas

Jarvis, M.; Harrison, C. M.; Mainieri,; Alexander, D. M.; Battaia, Fabrizio Arrigoni; Rivera, G. Calistro; Circosta, C.; Costa, Tiago; Breuck, C. De; Edge, Alastair; Girdhar, A.; Kakkad, D.; Kharb, P.; Lansbury, G. B.; Molyneux, S. J.; Mukherjee, Dipanjan; Mullaney, James; Farina, Emanuele Paolo; Silpa, S.; Thomson, A. P.; Ward, Samuel Ruthven

doi:10.1093/mnras/stab549

Cited by 48 publications

(46 citation statements)

References 183 publications

(260 reference statements)

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“…Such nuclei are part of a large population of radio LLAGN and faint nuclear starbursts ( 10 17.6 W Hz −1 ). This result adds observational evidence that a large fraction of LLAGN (even RQ AGN) feature low-power galactic-scale jets (Webster et al 2021), which may have a tremendous impact on their hosts by continuously injecting energy, a fundamental ingredient for galaxy feedback (Morganti 2017;Jarvis et al 2019;Hardcastle & Croston 2020;Smith et al 2020b;Jarvis et al 2021;Venturi et al 2021), as supported by the state-of-the-art jet simulations (Massaglia et al 2016;Mukherjee et al 2018Mukherjee et al , 2020.…”

Section: The Lemmings Viewsupporting

confidence: 63%

LeMMINGs III. The e-MERLIN legacy survey of the Palomar sample: exploring the origin of nuclear radio emission in active and inactive galaxies through the [O iii] – radio connection

Baldi

Williams

Beswick

et al. 2021

Monthly Notices of the Royal Astronomical Society

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What determines the nuclear radio emission in local galaxies? To address this question, we combine optical [O iii] line emission, robust black hole (BH) mass estimates, and high-resolution e-MERLIN 1.5-GHz data, from the LeMMINGs survey, of a statistically complete sample of 280 nearby optically active (LINER and Seyfert) and inactive [H ii and absorption line galaxies (ALGs)] galaxies. Using [O iii] luminosity ($L_{\rm [O\, \small {III}]}$) as a proxy for the accretion power, local galaxies follow distinct sequences in the optical–radio planes of BH activity, which suggest different origins of the nuclear radio emission for the optical classes. The 1.5-GHz radio luminosity of their parsec-scale cores (Lcore) is found to scale with BH mass (MBH) and [O iii] luminosity. Below MBH ∼ 106.5 M⊙, stellar processes from non-jetted H ii galaxies dominate with $L_{\rm core} \propto M_{\rm BH}^{0.61\pm 0.33}$ and $L_{\rm core} \propto L_{\rm [O\, \small {III}]}^{0.79\pm 0.30}$. Above MBH ∼ 106.5 M⊙, accretion-driven processes dominate with $L_{\rm core} \propto M_{\rm BH}^{1.5-1.65}$ and $L_{\rm core} \propto L_{\rm [O\, \small {III}]}^{0.99-1.31}$ for active galaxies: radio-quiet/loud LINERs, Seyferts, and jetted H ii galaxies always display (although low) signatures of radio-emitting BH activity, with $L_{\rm 1.5\, GHz}\gtrsim 10^{19.8}$ W Hz−1 and MBH ≳ 107 M⊙, on a broad range of Eddington-scaled accretion rates ($\dot{m}$). Radio-quiet and radio-loud LINERs are powered by low-$\dot{m}$ discs launching sub-relativistic and relativistic jets, respectively. Low-power slow jets and disc/corona winds from moderately high to high-$\dot{m}$ discs account for the compact and edge-brightened jets of Seyferts, respectively. Jetted H ii galaxies may host weakly active BHs. Fuel-starved BHs and recurrent activity account for ALG properties. In conclusion, specific accretion–ejection states of active BHs determine the radio production and the optical classification of local active galaxies.

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Section: The Lemmings Viewsupporting

confidence: 63%

LeMMINGs III. The e-MERLIN legacy survey of the Palomar sample: exploring the origin of nuclear radio emission in active and inactive galaxies through the [O iii] – radio connection

Baldi

Williams

Beswick

et al. 2021

Monthly Notices of the Royal Astronomical Society

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“…A similar correlation has also been observed in radio-quiet sources using SDSS-measured [OIII] luminosities (Jarvis et al 2021). Here we investigate whether similar correlation exists in red geyser galaxies.…”

Section: Integrated Propertiessupporting

confidence: 79%

“…As reported in §5.1, 14 out of 28 (∼ 50%) sources showing resolved radio emission in LOFAR observations display a compact radio morphology. Although similar radio-quiet compact sources hosting radio AGN have been observed to host small-scale (∼ 1 kpc) radio jets in higher spatial resolution (< 1 ) radio observations in previous studies (Jarvis et al 2019(Jarvis et al , 2021Venturi et al 2021;Panessa et al 2019;Webster et al 2021), the presence of resolved radio jets in the red geyser sample is observed to be quite rare with the current 5 resolution.…”

Section: Integrated Propertiesmentioning

confidence: 54%

“…Low-luminosity jets from radio-quiet AGN are the most plausible explanation for the observed low power radio emission in our red geyser targets. Sufficiently deep and high resolution radio observations have been able to identify smallscale radio jets in several "radio-quiet" quasars and Seyfert galaxies (Gallimore et al 2006;Jarvis et al 2019Jarvis et al , 2021Venturi et al 2021). Our sample of radio-quiet red geysers have many properties in common with jetted compact radio galaxies similar to those in Kimball et al (2011); ; Jarvis et al (2019).…”

Section: Discussionmentioning

confidence: 84%

“…In addition to using the criterion of Xu et al (1999), we compute the commonly used radio-loudness parameter R, the ratio of radio to optical brightness (Kellermann et al 1989), to differentiate between "radio-loud" and "radio-quiet" sources in our sample. Similar to Ivezić et al (2002) and Jarvis et al (2021), we calculate R using the radio flux density at 1.4 GHz calculated in a similar way as mentioned above, and the SDSS i-band apparent magnitude using the following equation:…”

Section: Radio Detection and Characterizationmentioning

confidence: 99%

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Radio Morphology of Red Geysers

Roy

Moravec

Bundy

et al. 2021

ApJ

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We present 150 MHz, 1.4 GHz, and 3 GHz radio imaging (LoTSS, FIRST, and VLASS) and spatially resolved ionized gas characteristics (SDSS IV-MaNGA) for 140 local (z < 0.1) early-type red geyser galaxies. These galaxies have a low star formation activity (with a star formation rate, SFR, ∼ 0.01 M ⊙ yr−1), but show unique extended patterns in spatially resolved emission-line maps that have been interpreted as large-scale ionized winds driven by active galactic nuclei (AGN). In this work, we confirm that red geysers host low-luminosity radio sources (L 1.4GHz ∼ 1022 WHz −1). Out of 42 radio-detected red geysers, 32 are spatially resolved in LoTSS and FIRST, with radio sizes varying between ∼5–25 kpc. Three sources have radio sizes exceeding 40 kpc. A majority display a compact radio morphology and are consistent with either low-power compact radio sources (FR0 galaxies) or radio-quiet quasars. They may be powered by small-scale AGN-driven jets that remain unresolved at the current 5″ resolution of radio data. The extended radio sources, not belonging to the “compact” morphological class, exhibit steeper spectra with a median spectral index of −0.67, indicating the dominance of lobed components. The red geysers hosting extended radio sources also have the lowest specific SFRs, suggesting they either have a greater impact on the surrounding interstellar medium or are found in more massive halos on average. The degree of alignment of the ionized wind cone and the extended radio features are either 0° or 90°, indicating possible interaction between the interstellar medium and the central radio AGN.

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Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies

Magliocchetti

2022

Astron Astrophys Rev

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Despite their relative sparseness, during the recent years it has become more and more clear that extragalactic radio sources (both AGN and star-forming galaxies) constitute an extremely interesting mix of populations, not only because of their intrinsic value, but also for their fundamental role in shaping our universe the way we see it today. Indeed, radio-active AGN are now thought to be the main players involved in the evolution of massive galaxies and clusters. At the same time, thanks to the possibility of being observed up to very high redshifts, radio galaxies can also provide crucial information on both the star-formation history of our universe and on its large-scale structure properties and their evolution. In the light of present and forthcoming facilities such as LOFAR, MeerKAT and SKA that will probe the radio sky to unprecedented depths and widths, this review aims at providing the current state of the art on our knowledge of extragalactic radio sources in connection with their hosts, large-scale environments and cosmological context.

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The quasar feedback survey: discovering hidden Radio-AGN and their connection to the host galaxy ionized gas

Cited by 48 publications

References 183 publications

LeMMINGs III. The e-MERLIN legacy survey of the Palomar sample: exploring the origin of nuclear radio emission in active and inactive galaxies through the [O iii] – radio connection

LeMMINGs III. The e-MERLIN legacy survey of the Palomar sample: exploring the origin of nuclear radio emission in active and inactive galaxies through the [O iii] – radio connection

Radio Morphology of Red Geysers

Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies

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