The nature of compact radio sources: the case of FR 0 radio galaxies
RD Baldi - The Astronomy and Astrophysics Review, 2023 - Springer
Radio-loud compact radio sources (CRSs) are characterised by morphological compactness
of the jet structure centred on the active nucleus of the galaxy. Most of the local elliptical …
of the jet structure centred on the active nucleus of the galaxy. Most of the local elliptical …
Radio jets from AGNs in dwarf galaxies in the COSMOS survey: mechanical feedback out to redshift∼ 3.4
M Mezcua, H Suh, F Civano - Monthly Notices of the Royal …, 2019 - academic.oup.com
Dwarf galaxies are thought to host the remnants of the early Universe seed black holes
(BHs) and to be dominated by supernova feedback. However, recent studies suggest that …
(BHs) and to be dominated by supernova feedback. However, recent studies suggest that …
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] …
RD Baldi, DRA Williams, RJ Beswick… - Monthly Notices of …, 2021 - academic.oup.com
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 …
combine optical [O iii] line emission, robust black hole (BH) mass estimates, and high …
Unravelling the origin of extended radio emission in narrow-line Seyfert 1 galaxies with the JVLA
Narrow-line Seyfert 1 galaxies (NLS1s) are believed to be active galactic nuclei (AGN) in the
early stages of their evolution. Several dozen of them have been found to host relativistic …
early stages of their evolution. Several dozen of them have been found to host relativistic …
LeMMINGs – II. The e-MERLIN legacy survey of nearby galaxies. The deepest radio view of the Palomar sample on parsec scale
RD Baldi, DRA Williams, IM McHardy… - Monthly Notices of …, 2021 - academic.oup.com
We present the second data release of high-resolution (≤ 0.2 arcsec) 1.5-GHz radio images
of 177 nearby galaxies from the Palomar sample, observed with the e-MERLIN array, as part …
of 177 nearby galaxies from the Palomar sample, observed with the e-MERLIN array, as part …
Evidence for Low-power Radio Jet–ISM Interaction at 10 pc in the Dwarf AGN Host NGC 4395
Black-hole-driven outflows in galaxies hosting active galactic nuclei (AGN) may interact with
their interstellar medium (ISM) affecting star formation (SF). Such feedback processes …
their interstellar medium (ISM) affecting star formation (SF). Such feedback processes …
Hard-X-ray-selected active galactic nuclei–II. Spectral energy distributions in the 5–45 GHz domain
F Panessa, E Chiaraluce, G Bruni… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT A wide-frequency radio study of active galactic nuclei (AGN) is crucial to
evaluate the intervening radiative mechanisms responsible for the observed emission and …
evaluate the intervening radiative mechanisms responsible for the observed emission and …
BAT AGN spectroscopic survey-XV: the high frequency radio cores of ultra-hard X-ray selected AGN
KL Smith, RF Mushotzky, M Koss… - Monthly Notices of …, 2020 - academic.oup.com
We have conducted 22 GHz radio imaging at 1 arcsec resolution of 100 low-redshift AGN
selected at 14–195 keV by the Swift-BAT. We find a radio core detection fraction of 96 per …
selected at 14–195 keV by the Swift-BAT. We find a radio core detection fraction of 96 per …
FRAMEx. III. Radio Emission in the Immediate Vicinity of Radio-quiet AGNs
OI Shuvo, MC Johnson, NJ Secrest… - The Astrophysical …, 2022 - iopscience.iop.org
We present follow-up results from the first Fundamental Reference AGN Monitoring
Experiment (FRAMEx) X-ray/radio snapshot program of a volume-complete sample of local …
Experiment (FRAMEx) X-ray/radio snapshot program of a volume-complete sample of local …
Is there a sub-parsec-scale jet base in the nearby dwarf galaxy NGC 4395?
ABSTRACT NGC 4395 is a dwarf galaxy at a distance of about 4.3 Mpc (scale:∼ 0.021 pc
mas− 1). It hosts an intermediate-mass black hole (IMBH) with a mass between∼ 104 and∼ …
mas− 1). It hosts an intermediate-mass black hole (IMBH) with a mass between∼ 104 and∼ …