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The nearby galaxy NGC 3115 contains a known radio-emitting, low-luminosity active galactic nucleus (AGN), and was recently claimed to host a candidate AGN displaced 14.3 pc from the galaxy's optical photocenter. Our goal is to understand…

Astrophysics of Galaxies · Physics 2019-04-03 Megan L. Jones , Sarah Burke-Spolaor , Kristina Nyland , Joan M. Wrobel

We analyze an optical data cube of the nuclear region of NGC 3621, taken with the integral field unit of the Gemini Multi-object Spectrograph. We found that the previously detected central line emission in this galaxy actually comes from a…

Astrophysics of Galaxies · Physics 2016-02-09 R. B. Menezes , J. E. Steiner , Patrícia da Silva

We present a spectroscopic and imaging study of an abnormal active galactic nucleus (AGN), 2MASX J00423991+3017515. This AGN is newly identified in the hard X-rays by the Swift BAT All-Sky survey and found in an edge-on disk galaxy…

Astrophysics of Galaxies · Physics 2021-03-17 J. Drew Hogg , Laura Blecha , Christopher S. Reynolds , Krista Lynne Smith , Lisa M. Winter

We report the discovery of an Active Galactic Nucleus (AGN) in the nearby SAd galaxy NGC 3621 using Spitzer high spectral resolution observations. These observations reveal the presence of [NeV] 14 um and 24 um emission which is centrally…

Astrophysics · Physics 2019-08-19 S. Satyapal , D. Vega , T. Heckman , B. O'Halloran , R. Dudik

The early-type galaxy NGC 3115, at a distance of 10.2 Mpc, hosts the nearest billion-solar-mass black hole. Wong et al. recently inferred a substantial Bondi accretion rate near the black hole. Bondi-like accretion is thought to fuel…

Astrophysics of Galaxies · Physics 2015-06-11 J. M. Wrobel , K. Nyland

NGC 3115 is the nearest galaxy hosting a billion solar mass black hole and is also a low-luminosity active galactic nucleus (LLAGN). X-ray observations of this LLAGN are able to spatially resolve the hot gas within the sphere of…

Astrophysics of Galaxies · Physics 2018-01-31 Ivan Almeida , Rodrigo Nemmen , Ka-Wah Wong , Qingwen Wu , Jimmy A. Irwin

A detailed study of the morphology of lenticular galaxies is an important way to understand how this type of galaxy formed and evolves over time. Decomposing a galaxy into its components (disc, bulge, bar, ...) allows recovering the colour…

A previous narrow-slit ($0.1$ arcsec) Hubble Space Telescope observation unveiled a broad relativistic H$\alpha$ profile in NGC3147, a low-luminosity ($\mathrm{L_{bol}}\sim10^{42}$ erg s$^{-1}$), low-Eddington ratio…

High Energy Astrophysical Phenomena · Physics 2022-09-07 Stefano Bianchi , Marco Chiaberge , Ari Laor , Robert Antonucci , Atharva Bagul , Alessandro Capetti

We report the detection of a weak X-ray point source coincident with the nucleus of the bulgeless disk galaxy NGC 3621, recently discovered by Spitzer to display high ionization mid-infrared lines typically associated with AGN. These…

High Energy Astrophysical Phenomena · Physics 2009-07-24 M. Gliozzi , S. Satyapal , M. Eracleous , L. Titarchuk , C. C. Cheung

We present the {\it Spitzer} Space Telescope InfraRed Array Camera (IRAC) and Multiband Imaging Photometer (MIPS) observations of the elliptical galaxy NGC 315. After removal of the host galaxy's stellar emission, we detected for the first…

Astrophysics · Physics 2009-11-13 Qiusheng Gu , J. -S. Huang , G. Wilson , G. Fazio

We present spectroscopic evidence for a low-luminosity, low-excitation active galactic nucleus (AGN) in NGC 1042, powered by an intermediate-mass black hole. These findings are significant in that the AGN is coincident with a compact star…

The Seyfert galaxy NGC 5515 has double-peaked narrow-line emission in its optical spectrum, and it has been suggested that this could indicate that it has two active nuclei. We observed the source with high resolution Very Long Baseline…

Astrophysics of Galaxies · Physics 2015-06-22 K. É. Gabányi , S. Frey , T. Xiao , Z. Paragi , T. An , E. Kun , L. Á. Gergely

We report on the changing-look nature of the active galactic nucleus (AGN) in the galaxy NGC 4156, as serendipitously discovered thanks to data acquired in 2019 at the Telescopio Nazionale Galileo (TNG) during a students' observing…

Type 2 active galactic nuclei (AGN) show signatures of accretion onto a supermassive black hole through strong, high-ionization, narrow emission lines extended on scales of 100s to 1000s of parsecs, but they lack the broad emission lines…

High Energy Astrophysical Phenomena · Physics 2022-09-21 M. Lynne Saade , Murray Brightman , Daniel Stern , Matthew A. Malkan , Javier A. Garcia

We have obtained new spectropolarimetric observations at visible wavelengths of the changing-look active galactic nucleus (AGN) Mrk 1018. The AGN direct spectrum shows an extremely weak continuum with faint broad H$\beta$ and H$\alpha$…

Astrophysics of Galaxies · Physics 2021-01-04 Damien Hutsemékers , Beatriz Agís González , Frédéric Marin , Dominique Sluse

As a first step of a program aimed to the detection of dark matter (or radial variations of M/L) in early-type galaxies, we report deep spectroscopic observations of the bulge-dominated edge-on S0 galaxy NGC 3115, made at ESO, La Silla,…

Astrophysics · Physics 2007-05-23 M. Capaccioli , E. Cappellaro , E. V. Held , M. Vietri

NGC 4527 is a nearby edge-on spiral galaxy with both starburst and AGN features, hosting a LINER nucleus. We present a radio study of the large-scale structure and nuclear region of this galaxy, based on new uGMRT observations at 700 and…

Astrophysics of Galaxies · Physics 2025-09-03 C. A. Galante , G. E. Romero , J. Saponara , P. Benaglia

We present evidence of the co-existence of either an AGN or an ultraluminous X-ray source (ULX), together with a young super stellar cluster in the 3 central parsecs of NGC4303. The galaxy contains a low luminosity AGN and hosts a number of…

In this paper, we report a detailed study with a variety of data from optical, near-infrared, X-ray, and radio telescopes of the nuclear region of the galaxy NGC 613 with the aim of understanding its complexity. We detected an extended…

Astrophysics of Galaxies · Physics 2020-01-22 Patrícia da Silva , Roberto B. Menezes , João E. Steiner
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