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Published in 2025 at "Research in Astronomy and Astrophysics"
DOI: 10.1088/1674-4527/ade9e9
Abstract: We estimated radiative efficiency, spin and supermassive black hole (SMBH) mass values for sample of 33 distant low luminosity active galactic nuclei (AGNs). The distribution of the estimated spin values (majority of objects have a…
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Keywords:
low luminosity;
distant low;
smbhs distant;
spin ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa083
Abstract: The majority of the activity around nearby (z ~ 0) supermassive black holes is found in low-luminosity active galactic nuclei (LLAGN), the most of them being classified as low ionization nuclear emission regions. Although these…
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Keywords:
gamma ray;
active galactic;
luminosity active;
gamma ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa1762
Abstract: One distinctive feature of low-luminosity active galactic nuclei (LLAGN) is the relatively weak reflection features they may display in the X-ray spectrum, which can result from the disappearance of the torus with decreasing accretion rates.…
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Keywords:
xmm newton;
reflection;
ngc 3718;
low luminosity ... See more keywords
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Published in 2025 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staf893
Abstract: We present optical-ultraviolet photometry and optical spectra for the type II supernova (SN) 2022acko. The spectroscopic observations span phases from ∼ 1.5 to ∼ 60 days after the explosion, while the light curve was observed up…
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Keywords:
low luminosity;
circumstellar interaction;
emission;
2022acko low ... See more keywords
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Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stx3259
Abstract: We analysed the four-decades-long X-ray light curve of the low-luminosity active galactic nucleus (LLAGN) NGC 7213 and discovered a fast-rise-exponential-decay (FRED) pattern, i.e. the X-ray luminosity increased by a factor of $\approx 4$ within 200d,…
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Keywords:
decades long;
fast rise;
luminosity;
ngc 7213 ... See more keywords
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Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty1581
Abstract: We present an analysis of a new sample of type II core-collapse supernovae (SNe II) occurring within low-luminosity galaxies, comparing these with a sample of events in brighter hosts. Our analysis is performed comparing SN…
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Keywords:
host galaxies;
type supernovae;
luminosity;
host ... See more keywords
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Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty564
Abstract: We present Very Long Baseline Interferometry observations of a faint and low-luminosity ($L_{\rm 1.4 GHz} < 10^{27}~\mbox{W Hz}^{-1}$) Gigahertz-Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) sample. We select eight sources from deep radio observations…
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Keywords:
radio;
luminosity;
peaked spectrum;
spectrum ... See more keywords
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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz3474
Abstract: NGC 3115 is known as the low-luminosity active galactic nucleus that hosts the nearest (z ∼ 0.002) billion-solar-mass supermassive black hole (∼1.5 × 109 M⊙). Its Bondi radius rB (∼3.6 arcsec) can be readily resolved with Chandra, which…
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Keywords:
active galactic;
radius;
gas;
luminosity active ... 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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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz716
Abstract: The feeble radiative efficiency characteristic of Low-Luminosity Active Galactic Nuclei (LLAGNs) is ascribed to a sub-Eddington accretion rate, typically at log (Lbol/Ledd) ≲ −3. At the finest angular resolutions that are attainable nowadays using mid-infrared (mid-IR)…
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Keywords:
ngc 1052;
continuum;
compact jet;
low luminosity ... See more keywords
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Published in 2025 at "Universe"
DOI: 10.3390/universe11030082
Abstract: In this work, we study the Coma cluster, one of the richest and most well-known systems at low redshifts, to explore the importance of low-flux objects in the identification of cluster substructures. In addition, we…
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Keywords:
role;
luminosity galaxies;
low luminosity;
galaxy clusters ... See more keywords