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相关论文: Nuclear/Circumnuclear Starbursts and Active Galact…

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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 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

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

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

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

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

We have analyzed the frequency and properties of the nuclear activity in a sample of galaxies with circumnuclear rings and spirals (CNRs). This sample was compared with a control sample of galaxies with very similar global properties but…

天体物理学 · 物理学 2007-05-23 R. J. Diaz , M. P. Aguero , H. Dottori

We have analyzed the frequency and properties of the nuclear activity in a sample of galaxies with circumnuclear rings and spirals (CNRs). This sample was compared with a control sample of galaxies with very similar global properties but…

星系天体物理 · 物理学 2016-05-17 M. P. Aguero , R. J. Diaz , H. Dottori

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

We analyse star formation in the nuclei of 9 Seyfert galaxies at spatial resolutions down to 0.085arcsec, corresponding to length scales of less than 10pc in some objects. Our data were taken mostly with the near infrared adaptive optics…

天体物理学 · 物理学 2009-11-13 R. Davies , F. Mueller Sanchez , R. Genzel , L. Tacconi , E. Hicks , S. Friedrich , A. Sternberg

We assess the potential of nuclear starburst disks to obscure the Seyfert-like AGN that dominate the hard X-ray background at z~1. Over 1200 starburst disk models, based on the theory developed by Thompson et al., are calculated for five…

天体物理学 · 物理学 2009-11-13 D. R. Ballantyne

We explore the formation of dusty gas walls induced by a circumnuclear starburst around an AGN. We concentrate our attention on the role of the radiation force by a starburst as well as an AGN, where the effects of optical depth of dusty…

天体物理学 · 物理学 2009-11-06 Ken Ohsuga , Masayuki Umemura

We compare the arcsecond-scale circumnuclear radio continuum properties between five Seyfert and five starburst galaxies, concentrating on the search for any structures that could imply a spatial or causal connection between the nuclear…

天体物理学 · 物理学 2008-11-26 Seppo Laine , Jari K. Kotilainen , Juha Reunanen , Stuart D. Ryder , Rainer Beck

We report on infrared K- (2-2.5 micron) and L-band (2.8-4.1 micron) slit spectroscopy of 23 Seyfert 1 galaxies in the CfA and 12 micron samples. A polycyclic aromatic hydrocarbon (PAH) emission feature at 3.3 micron in the L band is…

天体物理学 · 物理学 2009-11-10 Masatoshi Imanishi , Keiichi Wada

There is considerable evidence that the circumnuclear regions of galaxies are intimately related to their host galaxies, most directly through their bars. There is also convincing evidence for relations between the properties of…

天体物理学 · 物理学 2016-01-27 Johan H. Knapen

We present near-infrared K- (1.9-2.5 micrometer) and L- (2.8-4.2 micrometer) band spectroscopy of 22 Seyfert nuclei. We use two methods to investigate the presence of nuclear starbursts: (1) the Polycyclic Aromatic Hydrocarbon (PAH)…

星系天体物理 · 物理学 2015-05-20 Nagisa Oi , Masatoshi Imanishi , Keisuke Imase

The large scale (~ 100 kpc) environments of Seyfert galaxies are not significantly different from those of non-Seyfert galaxies. In the context of the interaction model of the formation of active galactic nuclei (AGN), it has been proposed…

天体物理学 · 物理学 2009-10-31 Michael R. Corbin

We analyze X-ray spectra and images of a sample of Seyfert 2 galaxies that unambiguously contain starbursts, based on their optical and UV characteristics. Although all sample members contain active galactic nuclei (AGNs), supermassive…

天体物理学 · 物理学 2009-10-31 N. A. Levenson , K. A. Weaver , T. M. Heckman

Over the last five decades, AGN studies have produced a number of spectacular examples of synergies and multifaceted approaches in astrophysics. The field of AGN research now spans the entire spectral range and covers more than twelve…

天体物理学 · 物理学 2015-06-24 Andrei P. Lobanov , J. Anton Zensus

In a matched sample of Seyfert and quiescent galaxies we simultaneously probe the stellar and molecular gas kinematics from 1 kpc down to 50 pc with the aim of identifying the dynamical processes dictating black hole accretion rates. This…

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