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We present a statistical analysis of the connections between galactic bars, star formation, and active galactic nucleus (AGN) activity using 33,201 disk galaxies (0.01 < z < 0.05) from DESI DR1 cross-matched with Galaxy Zoo DESI. Based on…

星系天体物理 · 物理学 2026-05-07 Jianfei Liu , Zhimin Zhou

The role of large-scale bars in the fuelling of active galactic nuclei (AGN) is still debated, even as evidence mounts that black hole growth in the absence of galaxy mergers cumulatively dominated and may substantially influence disc…

We explore the significance of bars in triggering central star formation (SF) and AGN activity for spiral galaxy evolution using a volume-limited sample with $0.020<z<0.055$, $M_{\rm r}<-19.5$, and $\sigma>70\rm km s^{-1}$ selected from…

星系天体物理 · 物理学 2020-09-09 Minbae Kim , Yun-Young Choi , Sungsoo S. Kim

The high luminosity displayed by an active galactic nucleus (AGN) requires that gas be transported to the centre of the galaxy by some mechanism. Bar-driven processes are often pointed out in this context and a number of studies have…

星系天体物理 · 物理学 2022-05-11 Luiz A. Silva-Lima , Lucimara P. Martins , Paula R. T. Coelho , Dimitri A. Gadotti

Despite the evidence that supermassive black holes (SMBHs) co-evolve with their host galaxy, and that most of the growth of these SMBHs occurs via merger-free processes, the underlying mechanisms which drive this secular co-evolution are…

We investigate the connection between the presence of bars and AGN activity, using a volume-limited sample of $\sim$9,000 late-type galaxies with axis ratio $b/a>0.6$ and $M_{r} < -19.5+5{\rm log}h$ at low redshift ($0.02\le z\lesssim…

宇宙学与河外天体物理 · 物理学 2015-06-04 Gwang-Ho Lee , Jong-Hak Woo , Myung Gyoon Lee , Ho Seong Hwang , Jong Chul Lee , Jubee Sohn , Jong Hwan Lee

We present empirical constraints on the influence of stellar bars on the fueling of active galactic nuclei (AGNs) out to z=0.84 using a sample of X-ray-selected AGNs hosted in luminous non-interacting face-on and moderately inclined disk…

星系天体物理 · 物理学 2015-06-22 Mauricio Cisternas , Kartik Sheth , Mara Salvato , Johan H. Knapen , Francesca Civano , Paola Santini

With the aim of assessing the effects of bars on active galactic nuclei (AGN), we present an analysis of host characteristics and nuclear activity of AGN galaxies with and without bars selected from the Sloan Digital Sky Survey Data Release…

宇宙学与河外天体物理 · 物理学 2015-06-12 Sol Alonso , Georgina Coldwell , Diego Garcia Lambas

In an effort to elevate to higher grounds our understanding on the impact of the formation and evolution of bars in the formation and evolution of galaxies, we have developed a diagnostic tool to distinguish between recently formed and…

天体物理学 · 物理学 2009-11-10 Dimitri A. Gadotti , Ronaldo E. de Souza

We study the influence of the presence of a strong bar in disc galaxies which host an active galactic nucleus (AGN). Using data from the Sloan Digital Sky Survey and morphological classifications from the Galaxy Zoo 2 project, we create a…

Bars are considered an efficient mechanism for transporting gas toward the central regions of galaxies, potentially enhancing nuclear activity. However, the extent to which bars influence active galactic nuclei (AGNs), and whether their…

星系天体物理 · 物理学 2025-06-02 V. Marels , V. Mesa , M. Jaque Arancibia , S. Alonso , G. Coldwell , G. Damke , V. Contreras Rojas

Galactic bars are often suspected to be a channel of gas inflow to the galactic center and trigger central star formation and active galactic nuclei (AGN) activity. However, the current status on this issue based on empirical studies is…

星系天体物理 · 物理学 2015-06-03 Seulhee Oh , Kyuseok Oh , Sukyoung K. Yi

We review general observational properties of bars in galaxies, and relations between bars, their dynamics, and (circum)nuclear activity. We consider new measurements of bar fractions and of the distribution of bars with host type, bar…

天体物理学 · 物理学 2009-09-25 Johan H. Knapen

We investigate the role of galactic bars in fuelling and triggering Active Galactic Nucleus (AGN) in disc galaxies up to $z\sim 0.8$. We utilise a Deep Learning model, fine-tuned on Galaxy Zoo volunteer classifications, to identify…

星系天体物理 · 物理学 2026-03-04 A. La Marca , M. T. Nardone , L. Wang , B. Margalef-Bentabol , S. Kruk , S. C. Trager

Galactic bars are the most important driver of secular evolution in galaxies. They can efficiently drive gas into the central kiloparsec of galaxies, thus feed circumnuclear starbursts, and possibly help to fuel AGN. The connection between…

宇宙学与河外天体物理 · 物理学 2009-10-22 Lei Hao , Shardha Jogee , Fabio D. Barazza , Irina Marinova , Juntai Shen

We explore properties of barred active spiral galaxies in groups selected from the SDSS-DR7, with the aim of assessing the effects of bars on AGN and the role of the high density environment. We identified barred active galaxies that reside…

星系天体物理 · 物理学 2015-06-23 Sol Alonso , Georgina Coldwell , Diego García Lambas

Aims: To unveil the influence of galaxy-galaxy interactions on material transport driven by galactic bars towards the central regions of active galactic nuclei (AGN) galaxies and assess the efficiency of the combined mechanisms of…

星系天体物理 · 物理学 2024-09-04 Sol Alonso , Matias Vera-Rueda , Georgina Coldwell , Fernanda Duplancic , Valeria Mesa

It is still a matter of intense debate how supermassive black holes (SMBH) grow, and the role played by feedback from active galactic nuclei (AGN) in the co-evolution of SMBHs and galaxies. To test the coevolution proposed by theoretical…

星系天体物理 · 物理学 2022-11-30 George Mountrichas , Francesco Shankar

Aims. With the aim of performing a suitable comparison of the internal process of galactic bars with respect to the external effect of interactions on driving gas toward the inner most region of the galaxies, we explored the efficiency of…

星系天体物理 · 物理学 2018-10-31 Sol Alonso , Georgina Coldwell , Fernanda Duplancic , Valeria Mesa , Diego G. Lambas

We analyse the properties of strongly barred disc galaxies using the TNG100 simulation, a cosmological hydrodynamical realisation of the IllustrisTNG suite. We identify 270 disc galaxies at $z=0$ in the stellar mass range…

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