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(Abridged). We present new high spatial resolution narrowband imaging observations of extraplanar diffuse ionized gas (eDIG) in four late-type, actively star forming edge-on spirals, obtained with ACS on-board HST. Our F658N (H-alpha)…

Astrophysics · Physics 2008-04-25 Joern Rossa , Michael Dahlem , Ralf-Juergen Dettmar , Roeland P. van der Marel

We present an analysis of the active galaxy SDSS J131642.90+175332.5, which is remarkable because all of its narrow emission lines are double-peaked, and because it additionally shows an extra broad component (FHWM ~ 1400 km/s) in most of…

Astrophysics of Galaxies · Physics 2015-05-14 Dawei Xu , S. Komossa

We identify a fading AGN SDSS J220141.64+115124.3 from the internal Product Launch-11 (MPL-11) in Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey. The central region with a projected radius of $\sim$2.4 kpc is…

Astrophysics of Galaxies · Physics 2024-03-15 Hao Mo , Yan-Mei Chen , Zhi-Yun Zhang , Alexei Moiseev , Dmitry Bizyaev , Yong Shi , Qiu-Sheng Gu , Min Bao , Xiao Cao , Song-Lin Li

We present the properties of the central supermassive black holes and the host galaxies of the interacting object SDSSJ134420.86+663717.8. We obtained optical long slit spectroscopy data from the Large Binocular Telescope (LBT) using the…

We present long-slit HST/STIS measurements of the ionized-gas kinematics in the nucleus of three disk galaxies, namely NGC 2179, NGC 4343, NGC 4435. The sample galaxies have been selected on the basis of their ground-based spectroscopy, for…

Astrophysics · Physics 2009-11-10 L. Coccato , E. Dalla Bonta' , M. Sarzi , A. Pizzella , E. M. Corsini , F. Bertola

The interaction between Active Galactic Nuclei (AGN) and their host galaxies is scarcely resolved. Narrow-line Seyfert 1 (NLS1) galaxies are believed to represent AGN at early stages of their evolution and allow to observe AGN feeding and…

We explore the gas ionization and kinematics, as well as the optical--IR spectral energy distributions for UGC 11185, a nearby pair of merging galaxies hosting obscured active galactic nuclei (AGNs), also known as SDSS J181611.72+423941.6…

As hybrids of narrow-line Seyfert 1 (NLS1) galaxies and blazars, {\gamma}-ray emitting NLS1s are important probes of jet physics in the high Eddington-ratio regime. Only very few of them are known to date; the majority of them below…

Astrophysics of Galaxies · Physics 2019-06-12 Su Yao , S. Komossa , Wen-Juan Liu , Weimin Yi , Weimin Yuan , Hongyan Zhou , Xue-Bing Wu

We present a $z = 0.94$ quasar, SDSS J004846.45-004611.9, discovered in the SDSS-III BOSS survey. A visual analysis of this spectrum reveals highly broadened and blueshifted narrow emission lines, in particular [Ne~V]$\lambda3426$ and…

We present a photometric FUV to Ks-band study of the field around quasar SDSS J092712.65+294344.0. The SDSS spectrum of this object shows various emission lines with two distinct redshifts, at z=0.699 and z=0.712. Because of this peculiar…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 R. Decarli , M. T. Reynolds , M. Dotti

Narrow Line Seyfert 1 galaxies (NLS1s) are intriguing due to their continuum as well as emission line properties. The observed peculiar properties of the NLS1s are believed to be due to accretion rate close to Eddington limit. As a…

Astrophysics · Physics 2016-08-30 Smita Mathur

The optically variable source SDSS J124602.54+011318.8 first appears in Sloan Digital Sky Survey (SDSS) data as a bright point source with nonstellar colors. Subsequent SDSS imaging and spectroscopy showed that the point source declined or…

Astrophysics · Physics 2009-11-07 Avishay Gal-Yam , Eran O. Ofek , Alexei V. Filippenko , Ryan Chornock , Weidong Li

We fit theoretical models to the emission-line spectra of 2766 Seyfert galaxies from the Sloan Digital Sky Survey (SDSS). The model line fluxes are derived by `mixing' photoionization model predictions of active galactic nucleus (AGN)…

Astrophysics of Galaxies · Physics 2018-07-11 Adam D. Thomas , Lisa J. Kewley , Michael A. Dopita , Brent A. Groves , Andrew M. Hopkins , Ralph S. Sutherland

Although thousands of galaxy mergers are known, only a handful of sub-kiloparsec-scale supermassive black hole (SMBH) pairs have been confirmed so far, leaving a huge gap between the observed and predicted numbers of such objects. In this…

In this paper we study the object SDSS J1130+0058 which is the only AGN known to have both double-peaked low-ionization broad emission lines, and also X-shaped radio structures. Emission from an accretion disk can reproduce the…

Astrophysics · Physics 2008-11-26 Xue-Guang Zhang , Dultzin-Hacyan D. , Ting-Gui Wang

"Green Bean" Galaxies (GBs) are the most [O III]-luminous type-2 active galactic nuclei (AGN) at z~0.3. However, their infrared luminosities reveal AGN in very low activity states, indicating that their gas reservoirs must be ionized by…

Astrophysics of Galaxies · Physics 2015-06-24 Rebecca L. Davies , Mischa Schirmer , James E. H. Turner

The merging of supermassive black holes (SMBHs) is a direct consequence of our hierarchical picture of galaxy evolution. It is difficult to track the merging process of SMBHs during mergers of galaxies as SMBHs are naturally difficult to…

Astrophysics of Galaxies · Physics 2020-07-22 B. Husemann , J. Heidt , A. De Rosa , C. Vignali , S. Bianchi , T. Bogdanović , S. Komossa , Z. Paragi

Observations with the James Webb Space Telescope (JWST) have uncovered a substantial population of high-redshift, broad-line active galactic nuclei (AGNs), whose properties challenge standard models of black hole growth and AGN emission. We…

Astrophysics of Galaxies · Physics 2026-02-25 Greta Zucchi , Xihan Ji , Piero Madau , Roberto Maiolino , Ignas Juodžbalis , Francesco D'Eugenio , Sophia Geris , Yuki Isobe

We report the identification of an unusual absorption line system in the quasar SDSS J080248.18$+$551328.9 and present a detailed study of the system, incorporating follow-up optical and NIR spectroscopy. A few tens of absorption lines are…

Narrow-line Seyfert 1 (NLS1) galaxies provide us with unique insights into the drivers of AGN activity under extreme conditions. Given their low black hole (BH) masses and near-Eddington accretion rates, they represent a class of galaxies…

High Energy Astrophysical Phenomena · Physics 2017-06-28 V. Karamanavis , E. Angelakis , S. Komossa , I. Myserlis , D. Blinov , J. A. Zensus