Results 41 to 50 of about 47,541 (242)

NuSTAR Observes Two Bulgeless Galaxies: No Hard X-Ray AGN Detected in NGC 4178 or J0851+3926

open access: yesThe Astrophysical Journal, 2023
The discovery over the last several decades of low- and moderate-luminosity active galactic nuclei (AGNs) in disk-dominated galaxies—which show no “classical” bulges—suggests that secular mechanisms represent an important growth pathway for supermassive ...
Ryan W. Pfeifle   +7 more
doaj   +1 more source

Radio Emission from Low-Luminosity Active Galactic Nuclei [PDF]

open access: yesInternational Astronomical Union Colloquium, 1998
AbstractMany nearby galaxies show optical evidence for low-luminosity AGNs that are far less luminous than classical Seyfert nuclei and QSOs. LINERs, the most common variety of such emission-line objects, comprise ~ 1/3 of nearby galaxies, and may serve as an important “missing link“ between normal and Seyfert galaxies.
Schuyler D. Van Dyk, Luis C. Ho
openaire   +1 more source

Calibrating Mg ii-based Black Hole Mass Estimators Using Low-to-high-luminosity Active Galactic Nuclei [PDF]

open access: yesAstrophysical Journal, 2020
We present single-epoch black hole mass (MBH) estimators based on the rest-frame ultraviolet (UV) Mg ii 2798 Å and optical Hβ 4861 Å emission lines. To enlarge the luminosity range of active galactic nuclei (AGNs), we combine the 31 reverberation-mapped ...
H. A. Le, J. Woo, Yongquan Xue
semanticscholar   +1 more source

The Clustering of Low‐Luminosity Active Galactic Nuclei [PDF]

open access: yesThe Astrophysical Journal, 2006
Based on the Sloan Digital Sky Survey (SDSS) DR2 sample, we present a multiparameter analysis of the spatial clustering of nearby active galactic nuclei (AGNs). Estimates of the redshift-space two-point correlation function reveal that Seyferts are less clustered than normal galaxies, while LINERs' clustering amplitude (s0) is consistent with that of ...
Anca Constantin, Michael S. Vogeley
openaire   +1 more source

NuStar Hard X-Ray View of Low-luminosity Active Galactic Nuclei: High-energy Cutoff and Truncated Thin Disk [PDF]

open access: yesAstrophysical Journal, 2018
We report the analysis of simultaneous XMM-Newton+Nuclear Spectroscopic Telescope Array (NuSTAR) observations of two low-luminosity active galactic nuclei (LLAGNs), NGC 3998 and NGC 4579. We do not detect any significant variability in either source over
G. Younes   +7 more
semanticscholar   +1 more source

Variability-selected Low-luminosity Active Galactic Nuclei Candidates in the 7 Ms Chandra Deep Field-South [PDF]

open access: yesAstrophysical Journal, 2018
In deep X-ray surveys, active galactic nuclei (AGNs) with a broad range of luminosities have been identified. However, cosmologically distant low-luminosity AGN (LLAGN, erg s−1) identification still poses a challenge because of significant contamination ...
N. Ding   +15 more
semanticscholar   +1 more source

Do LINER 2 galaxies harbour low-luminosity active galactic nuclei? [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2001
We use ROSAT HRI spatial data and ASCA spectral measurements for a sample of seven nearby, early type spiral galaxies, to address the question of whether a low-luminosity Active Galactic Nucleus (LLAGN) is present in galaxies that have a LINER 2 classification.
Roberts, TP, Schurch, NJ, Warwick, RS
openaire   +3 more sources

X-Ray Flares in the Long-term Light Curve of Low-luminosity Active Galactic Nucleus M81*

open access: yesThe Astrophysical Journal, 2023
Most active galactic nuclei at the center of the nearby galaxies have supermassive black holes accreting at sub-Eddington rates through hot accretion flows or radiatively inefficient accretion flows, which efficiently produce jets.
Gunjan Tomar, Nayantara Gupta
doaj   +1 more source

X-Ray Observations of Low-Luminosity Active Galactic Nuclei [PDF]

open access: yesInternational Astronomical Union Colloquium, 1997
AbstractThrough X-ray observations with ASCA, low-luminosity active galactic nuclei have been found in at least seven near-by spiral galaxies. Some of them exhibit very intense, and possibly broad, Fe-K emission lines. Their time variability is relatively insignificant, in contrast to lowluminosity Seyfert galaxies.
K. Makishima   +3 more
openaire   +1 more source

THE CENTRAL MOLECULAR GAS STRUCTURE IN LINERS WITH LOW-LUMINOSITY ACTIVE GALACTIC NUCLEI: EVIDENCE FOR GRADUAL DISAPPEARANCE OF THE TORUS [PDF]

open access: yes, 2012
We present observations of the molecular gas in the nuclear environment of three prototypical low-luminosity active galactic nuclei (LLAGNs), based on VLT/SINFONI AO-assisted integral-field spectroscopy of H2 1–0 S(1) emission at angular resolutions of ...
F. Muller-S'anchez   +11 more
semanticscholar   +1 more source

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