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相关论文: The Connection Between Barstrength and Circumnucle…

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The inner regions of barred galaxies contain substructures such as off-axis shocks, nuclear rings, and nuclear spirals. These substructure may affect star formation, and control the activity of a central black hole (BH) by determining the…

星系天体物理 · 物理学 2015-06-03 Woong-Tae Kim , Woo-Young Seo , James M. Stone , Doosoo Yoon , Peter J. Teuben

Several recent studies indicate that bulges are more complex than merely structureless relaxed stellar systems. We study the HST images of a sample of 130 nearby early type (S0-Sab) disc galaxies and detect pure structureless bulges with…

天体物理学 · 物理学 2008-10-16 Leonel Gutierrez , Antti Tamm , John Beckman , Louis Abramson , Peter Erwin , Melanie Guittet

Multicolour near IR photometry for a sample of 32 large barred spiral galaxies is presented. By applying ellipse fitting techniques, we identify significant isophote twists with respect to the primary bar axis in the nuclear regions of…

天体物理学 · 物理学 2015-06-24 M. Shaw , D. Axon , R. Probst , I. Gatley

Ring-shaped morphologies of nuclear star-forming regions within the central 40-200 pc of disk galaxies have been barely resolved so far in three composite Sy2 nuclei, the Sy2 Circinus galaxy and in three non-AGN galaxies. Such morphologies…

天体物理学 · 物理学 2009-11-13 S. Comerón , J. H. Knapen , J. E. Beckman , I. Shlosman

Many barred galaxies today harbor massive concentrations of gas in their centers, and some are known to possess supermassive black holes (SBHs) and their associated stellar cusps. Previous theoretical work has suggested that a bar in a…

天体物理学 · 物理学 2007-05-23 Juntai Shen , J. A. Sellwood

Fundamental properties of the extinction curve, like the slope in the rest-frame ultraviolet (UV) and the presence/absence of a broad absorption excess centred at 2175 A (the UV bump), are investigated for a sample of 108 massive,…

天体物理学 · 物理学 2009-11-13 S. Noll , D. Pierini , M. Pannella , S. Savaglio

We investigate the properties of massive, dense clouds formed in a barred galaxy and their possible relation to star formation, performing a two-dimensional hydrodynamical simulation with the gravitational potential obtained from the 2Mass…

星系天体物理 · 物理学 2015-06-05 M. Nimori , A. Habe , K. Sorai , Y. Watanabe , A. Hirota , D. Namekata

We present photometric and morphological analyses of nuclear star clusters (NSCs) -- very dense, massive star clusters present in the central regions of most galaxies -- in a sample of 33 massive disk galaxies within 20 Mpc, part of the…

Through observations and modeling, we demonstrate how the recently discovered large-scale bar in NGC 5248 generates spiral structure which extends from 10 kpc down to 100 pc, fuels star formation on progressively smaller scales, and drives…

(Abridge) Bars are very common in the centre of the disc galaxies, and they drive the evolution of their structure. A volume-limited sample of 2106 disc galaxies extracted from the Sloan Digital Sky Survey Data Release 5 was studied to…

星系天体物理 · 物理学 2009-11-13 J. A. L. Aguerri , J. Mendez-Abreu , E. M. Corsini

We test ideas on fueling of galactic nuclei by bar-driven inflow by comparing the detection rate and intensity of nuclear H II regions and AGNs among barred and unbarred galaxies in a sample of over 300 spirals selected from our recent…

天体物理学 · 物理学 2009-10-30 Luis C. Ho , Alexei V. Filippenko , Wallace L. W. Sargent

The Seyfert galaxy NGC 1097 has an extended neutral hydrogen disk, a companion, a prominent bar and a luminous circumnuclear starburst "ring". Magnetic fields as revealed by nonthermal radio-continuum emissions correlate well with the…

天体物理学 · 物理学 2009-11-06 Yu-Qing Lou , ZuHui Fan , Chi Yuan , Stephane Leon

The presence of nuclear discs in barred disc galaxies has been demonstrated in studies on stellar structures and kinematics. It is thus imperative to establish their fundamental properties and scaling relations, which can help understanding…

星系天体物理 · 物理学 2025-09-19 Dimitri A. Gadotti , Camila de Sá-Freitas

We numerically study the origin of the multi-armed spiral structure observed in the circumnuclear gaseous mini-disks of nearby galaxies. We show that the presence of dust in such disks and its interaction with the gravitationally stable…

星系天体物理 · 物理学 2023-03-13 Roman Tkachenko , Vladimir Korchagin , Boris Jmailov

Subjective classification of spiral galaxies is not sufficient for studying the effect of bars on their physical characteristics. In reality the problem is to comprehend the complex correlations in a multivariate parametric space.…

星系天体物理 · 物理学 2021-04-13 Prasenjit Banerjee , Tanuka Chattopadhyay , Asis Kumar Chattopadhyay

We present multi-wavelength (interferometer and single-dish CO J=1-0, Halpha, broadband optical and near-infrared) observations of the classic barred spiral NGC 5383. We compare the observed central gas and dust morphology to the…

天体物理学 · 物理学 2009-10-31 Kartik Sheth , Michael W. Regan , Stuart N. Vogel , Peter J. Teuben

The first results of the observational program of the study of 2D-kinematics in double-barred galaxies are presented. We show that, for the main part of the sample, the inner bars do not affect the circumnuclear stellar kinematics.…

天体物理学 · 物理学 2007-05-23 A. V. Moiseev , J. R. Valdes , V. H. Chavushyan

We present broad-band (U, V, I,and H) and narrow-band(H-alpha+[N II] and Paschen-alpha) images of the circumnuclear starburst rings in two nearby spiral galaxies, NGC 1512 and NGC 5248, obtained with WFPC2 and NICMOS on HST. Combined with…

天体物理学 · 物理学 2009-11-06 Dan Maoz , Aaron J. Barth , Luis C. Ho , Amiel Sternberg , Alexei V. Filippenko

We investigate the formation of circumnuclear gas structures from the tidal disruption of molecular clouds in galactic nuclei, by means of smoothed particle hydrodynamics simulations. We model galactic nuclei as composed of a supermassive…

星系天体物理 · 物理学 2018-09-05 Alessandro A. Trani , Michela Mapelli , Alessandro Ballone