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Observations at ultraviolet, optical and near-infrared wavelengths have shown the existence of recent star formation in the nuclear regions of Seyfert 2 (Sy2) galaxies that suggest a connection between the Starburst and the Seyfert…

天体物理学 · 物理学 2007-05-23 Rosa M. Gonzalez Delgado

Active galaxies are often associated with starbursts, which are possible sources of fuelling for the nuclear black holes. By means of optical (3500-7500 A) spectroscopic and narrow-band photometric data (H_alpha+[NII]6548,6583 and…

天体物理学 · 物理学 2007-05-23 A. Romano , A. Rifatto , S. Ciroi , P. Rafanelli , M. Dopita

We report the transition towards a type 1 Seyfert experienced by the classical type 2 Seyfert nucleus in NGC 7582. The transition, found at most 20 days from its maximum peak, presents a unique opportunity to study these rare events in…

天体物理学 · 物理学 2009-10-31 Itziar Aretxaga , B. Joguet , D. Kunth , J. Melnick , R. J. Terlevich

We investigated the correlation between nuclear/circumnuclear starbursts around the active galactic nuclei (AGNs) and the AGN activities for 43 Seyfert galaxies in the CfA and 12 micron samples. We found that circumnuclear starburst…

天体物理学 · 物理学 2009-11-13 Yasuyuki Watabe , Nozomu Kawakatu , Masatoshi Imanishi

We examine the possibility of the active galactic nucleus (AGN) obscuration by dusty gas clouds that spurt out from circumnuclear starburst regions. For the purpose, the dynamical evolution of gas clouds is pursued, including the effects of…

天体物理学 · 物理学 2009-11-10 Yasuyuki Watabe , Masayuki Umemura

We present a large sample which contains 45 Seyfert 1 galaxies (Sy1s), 46 hidden broad-line region (HBLR) Seyfert 2 galaxies (Sy2s), 57 non-HBLR Sy2s, and 22 starburst galaxies to distinguish their properties and to seek the possible…

高能天体物理现象 · 物理学 2015-05-28 Yu-Zhong Wu , Yong-Heng Zhao , Xian-Min Meng

Nuclear stellar clusters are a common phenomenon in spirals and in starbursts galaxies, and they may be a natural consequence of the star formation processes in the central regions of galaxies. HST UV imaging of a few Seyfert 2 galaxies…

天体物理学 · 物理学 2015-05-13 R. M. González Delgado , V. Muñoz Marin , E. Pérez , H. Schmitt , R. Cid Fernandes

Active Galactic Nuclei (AGN) are known to show flux variability over all observable timescales and across the entire electromagnetic spectrum. Over the past decade, a growing number of sources have been observed to show dramatic flux and…

星系天体物理 · 物理学 2022-11-11 Claudio Ricci , Benny Trakhtenbrot

In this paper, we present our preliminary results on Seyfert galaxies with circumnuclear/nuclear starburst(SB) activity. We have searched the recent available literature and found 76 active galaxies with clear evidence of nuclear SB…

天体物理学 · 物理学 2007-05-23 Qiusheng Gu , D. Dultzin-Hacyan , J. A. de Diego

NGC 7582 was identified as a Starburst galaxy in the optical \cite[(Veron et al. 1981)]{Veron et al.(1981)} but its X-Ray emission is typical of a Seyfert 1 galaxy \cite[(Ward et al. 1978)]{Ward et al.(1978)}. We analyzed a datacube of this…

宇宙学与河外天体物理 · 物理学 2015-05-18 T. V. Ricci , J. E. Steiner , R. B. Menezes , A. Garcia-Rissmann , R. Cid Fernandes

High quality infrared spectra of active galaxies including the stellar absorption features of Si at 1.59 um, CO(6,3) at 1.62 um, and CO(2,0) at 2.29 um are used to measure the stellar mass to light ratio at 1.65 um (M_H/L) and investigate…

天体物理学 · 物理学 2007-05-23 E. Oliva , L. Origlia , R. Maiolino , A. F. M. Moorwood

Detailed modeling of the different regions of NGC 7130 is presented, accounting for its composite nature of AGN and starburst galaxy. Shock waves, created by stellar winds from hot massive stars and by supernova ejecta, are evident in the…

天体物理学 · 物理学 2009-11-07 M. Contini , M. Radovich , P. Rafanelli , G. M. Richter

Two major challenges to unification schemes for active galactic nuclei (AGN) are the existence of Narrow-Line Seyfert 1s (NLS1s) and the existence of changing-look (CL) AGNs. AGNs can drastically change their spectral appearance in the…

星系天体物理 · 物理学 2019-07-09 Victor L. Oknyansky , Konstantin L. Malanchev , C. Martin Gaskell

Although it is clear that the circumnuclear regions of galaxies are intimately related to their host galaxies, most directly through their bars, it remains unclear what exactly initiates and fuels nuclear stellar (starburst) and non-stellar…

天体物理学 · 物理学 2007-05-23 Johan H. Knapen

The evolutionary role of the so-called ``changing-look'' (CL) active galactic nucleus (AGN), which is characterized by spectral-type transitions within $\sim10$ yr, has been suggested in the past few years. By focusing on CL-AGNs having…

星系天体物理 · 物理学 2026-03-24 J. Wang , S. Jin , D. W. Xu , WeiKang Zheng , Thomas G. Brink , S. Komossa , 1 Alexei V. Filippenko , J. Y. Wei

Active Galactic Nuclei (AGN) have long been known to be variable, but the amplitude, timescale and nature of these changes can often differ dramatically from object to object. The richest source of information about the properties of AGN…

星系天体物理 · 物理学 2021-07-14 Hartmut Winkler

Active galactic nuclei (AGNs) exhibit variability across the entire electromagnetic spectrum with distinct flaring episodes at different frequencies. The high sensitivity and nearly uniform sky coverage of the Large Area Telescope on board…

高能天体物理现象 · 物理学 2022-03-02 Filippo D'Ammando

We present an analysis of 10 ks snapshot Chandra observations of 12 shocked post-starburst galaxies, which provide a window into the unresolved question of active galactic nuclei (AGN) activity in post-starburst galaxies and its role in the…

Swift has initiated a new era of understanding the extremes of active galactic nuclei (AGN) variability, their drivers and underlying physics. This is based on its rapid response, high sensitivity, good spatial resolution, and its ability…

高能天体物理现象 · 物理学 2015-02-25 S. Komossa , D. Grupe , R. Saxton , L. Gallo

Far-infrared flux densities are newly extracted from the IRAS database for the RSA and CfA complete samples of Seyfert galaxies. These data are used to classify the Seyfert galaxies into those where the far-infrared continuum emission is…

天体物理学 · 物理学 2016-08-30 H. Mouri , Y. Taniguchi
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