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Related papers: A Multi-Wavelength Analysis of NGC 4178: A Bulgele…

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Using high resolution Chandra data, we report the presence of a weak X-ray point source coincident with the nucleus of NGC 4178, a late-type bulgeless disk galaxy known to have high ionization mid-infrared (mid-IR) lines typically…

Astrophysics of Galaxies · Physics 2015-06-05 Nathan Secrest , Shobita Satyapal , Mario Gliozzi , C. C. Cheung , Anil Seth , Torsten Boeker

The discovery over the last several decades of moderate luminosity AGNs in disk-dominated galaxies - which show no "classical" bulges - suggests that secular mechanisms represent an important growth pathway for supermassive black holes in…

We have conducted a high-resolution spectroscopic study using Spitzer of 18 bulgeless (Sd/Sdm) galaxies that show no definitive signatures of nuclear activity in their optical spectra. This is the first systematic mid-IR search for weak or…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 S. Satyapal , T. Boeker , W. Mcalpine , M. Gliozzi , N. P. Abel , T. Heckman

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 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 are conducting a search for supermassive black holes (SMBHs) with masses below 10^7 M_sun by looking for signs of extremely low-level nuclear activity in nearby galaxies that are not known to be AGNs. Our survey has the following…

Astrophysics · Physics 2009-11-13 Himel Ghosh , Smita Mathur , Fabrizio Fiore , Laura Ferrarese

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…

We present X-ray observations of the ultraluminous infrared galaxy, UGC 5101, thought to contain a buried active galactic nucleus (AGN) based on observations in other wavebands. We detected an absorbed hard component at >3 keV, as well as…

Astrophysics · Physics 2009-11-10 Masatoshi Imanishi , Yuichi Terashima , Naohisa Anabuki , Takao Nakagawa

AGN bubbles could play an important role in accelerating high-energy CRs and galactic feedback. Only in nearby galaxies could we have high enough angular resolution in multi-wavelengths to study the sub-kpc environment of the AGN, where the…

High Energy Astrophysical Phenomena · Physics 2022-08-17 Jiang-Tao Li , Q. Daniel Wang , Theresa Wiegert , Joel N. Bregman , Rainer Beck , Ancor Damas-Segovia , Judith A. Irwin , Li Ji , Yelena Stein , Wei Sun , Yang Yang

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 present the Chandra discovery of soft diffuse X-ray emission in NGC 4151 (L[0.5-2keV]~10^{39} erg s$^{-1}$), extending ~2 kpc from the active nucleus and filling in the cavity of the HI material. The best fit to the X-ray spectrum…

We present a detailed X-ray analysis of 4C+55.16, an unusual and interesting radio galaxy, located at the centre of a cool core cluster of galaxies. 4C+55.16 is X-ray bright (L(cluster)~10^45 erg/s), radio powerful, and shows clear signs of…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 J. Hlavacek-Larrondo , A. C. Fabian , J. S. Sanders , G. B. Taylor

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 galaxy NGC 4418 contains one of the most compact obscured nuclei within a luminous infrared galaxy (LIRG) in the nearby Universe. This nucleus contains a rich molecular gas environment and an unusually high ratio of infrared to radio…

Astrophysics of Galaxies · Physics 2014-06-04 E. Varenius , J. E. Conway , I. Martí-Vidal , S. Aalto , R. Beswick , F. Costagliola , H. -R. Klöckner

NGC 4278, a Low-luminosity active galactic nucleus (AGN), is generally classified as a low-ionization nuclear emission line region (LINER). Recently, it has been reported to be associated with a very high energy $\gamma$-ray source 1LHAASO…

High Energy Astrophysical Phenomena · Physics 2024-08-13 Ji-Shun Lian , Jia-Xuan Li , Xin-Ke Hu , Ying-Ying Gan , Tan-Zheng Wu , Hai-Ming Zhang , Jin Zhang

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…

The Seyfert galaxy NGC 4151 has been imaged at resolution better than 0.1 pc using a VLBI array consisting of the VLBA and three 100m-class telescopes. A flat-spectrum 3-mJy source with a monochromatic radio power of ~10^{37} ergs/s has…

We present new HST NICMOS observations of NGC 4945, a starburst galaxy hosting a highly obscured active nucleus that is one of the brightest extragalactic sources at 100 keV. The HST data are complemented with ground based [FeII] line and…

NGC 3115 is an S0 galaxy that has always been considered to have a pure absorption-line spectrum. Some recent studies have detected a compact radio-emitting nucleus in this object, coinciding with the photometric center and with a candidate…

Astrophysics of Galaxies · Physics 2014-11-14 R. B. Menezes , J. E. Steiner , T. V. Ricci

We present XMM-Newton observations of the Chandra-detected nuclear X-ray source in NGC 4561. The hard X-ray spectrum can be described by a model composed of an absorbed power-law with Gamma= 2.5^{+0.4}_{-0.3}, and column density…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 C. Araya Salvo , S. Mathur , H. Ghosh , F. Fiore , L. Ferrarese
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