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Published in 2019 at "Nature Astronomy"
DOI: 10.1038/s41550-019-0765-4
Abstract: The central nuclei of galaxies, where supermassive black holes (SMBHs) are thought to reside, can experience phases of activity when they become active galactic nuclei (AGNs). An AGN can eject winds and jets and produce…
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Keywords:
emission;
active galactic;
radio;
galactic nuclei ... See more keywords
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Published in 2024 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stae1617
Abstract: Powerful supermassive black hole (SMBH) winds in the form of ultra-fast outflows (UFOs) are detected in the X-ray spectra of several active galactic nuclei (AGN) seemingly independently of their radio classification between radio quiet (RQ)…
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Keywords:
supermassive black;
smbh winds;
agn;
black hole ... See more keywords
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Published in 2024 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stae1861
Abstract: Measuring the environments of massive galaxies at high redshift is crucial to understanding galaxy evolution and the conditions that gave rise to the distribution of matter we see in the Universe today. While high-z radio…
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Keywords:
field;
quiet galaxies;
environments massive;
massive radio ... See more keywords
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Published in 2025 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staf1946
Abstract: We searched the Hubble Space Telescope Cosmic Origins Spectrograph archive for ultraviolet spectra of 428 AGN to identify intrinsic N v absorption systems. We filtered out Type 2 AGN, blazars, and spectra that do not cover…
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Keywords:
radio loud;
loud quasars;
radio;
intrinsic absorbers ... See more keywords
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Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty1802
Abstract: A small subset of optically selected radio-quiet quasars showing weak or no emission lines may turn out to be the elusive radio-quiet BL Lac objects, or simply be radio-quiet QSOs with a still-forming/shielded broad line…
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Keywords:
radio quiet;
line;
radio;
weak emission ... See more keywords
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1
Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz3384
Abstract: The main objective of this work is to establish and interpret the dominant spectral components and their differences in radio-loud (RL) and radio-quiet (RQ) AGN with very massive black holes, and accreting at moderate rates.…
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Keywords:
loud radio;
radio quiet;
quiet agn;
radio ... See more keywords
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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz595
Abstract: A strong effort has been devoted to understand the physical origin of radio emission from low-luminosity AGN (LLAGN), but a comprehensive picture is still missing. We used high-resolution ($\le$1 arcsec), multi-frequency (1.5, 5.5, 9 and…
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Keywords:
radio emission;
radio;
radio quiet;
low luminosity ... See more keywords
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3
Published in 2023 at "Monthly Notices of the Royal Astronomical Society: Letters"
DOI: 10.1093/mnrasl/slad051
Abstract: Measuring the proper motion of the emission component in radio-quiet quasars (RQQs) could help to distinguish between the origins of the radio emission and to understand whether the jet production mechanism is the same in…
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Keywords:
radio quiet;
1351 640;
motion;
jet ... See more keywords
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Published in 2024 at "Frontiers in Astronomy and Space Sciences"
DOI: 10.3389/fspas.2024.1530392
Abstract: Active galactic nuclei (AGN) are powerful sources of panchromatic radiation. All AGN emit in X-rays, contributing around 5%–10% of the AGN bolometric luminosity. The X-ray emitting region, popularly known as the corona, is geometrically and…
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Keywords:
agn;
active galactic;
coronal emission;
galactic nuclei ... See more keywords