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相关论文: The Relative Role of Bars and Environments in AGN …

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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

Stellar bars are a common feature in massive disc galaxies. On a theoretical ground, the response of gas to a bar is generally thought to cause nuclear starbursts and, possibly, AGN activity once the perturbed gas reaches the central…

星系天体物理 · 物理学 2015-10-28 R. Fanali , M. Dotti , D. Fiacconi , F. Haardt

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

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

To investigate the role of bars in the chemical evolution of isolated disc galaxies, we performed a series of 39 gas dynamical simulations of isolated barred and unbarred galaxies with various masses, initial gas fractions, and AGN feedback…

星系天体物理 · 物理学 2018-05-02 Hugo Martel , Christian Carles , Fidèle Robichaud , Sara L. Ellison , David J. Williamson

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

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

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

[Abridged] We present an analysis of optical spectroscopically-identified AGN to M*+1 in a sample of 6 self-similar SDSS galaxy clusters at z=0.07. These clusters are specifically selected to lack significant substructure at bright limits…

宇宙学与河外天体物理 · 物理学 2015-06-12 K. A. Pimbblet , S. S. Shabala , C. P. Haines , A. Fraser-McKelvie , D. J. E. Floyd

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

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 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

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

What triggers AGN in some galaxies and what role does this brief period of activity play in the overall evolution of galaxies are still open questions. This paper explores whether or not the local, on scales of $\approx$1\,Mpc, galaxy…

星系天体物理 · 物理学 2025-10-03 Jason Reeves , Anna Sajina , Henry Adair , Duncan Farrah , Mark Lacy

There is compelling evidence that active galactic nuclei (AGNs) in high-density regions have undergone a different evolution than their counterparts in the field, indicating that they are strongly affected by their environment. To…

星系天体物理 · 物理学 2024-02-06 E. Koulouridis , A. Gkini , E. Drigga

Galaxy-galaxy interactions and large scale galaxy bars are usually considered as the two main mechanisms for driving gas to the centres of galaxies. By using large samples of galaxy pairs and visually classified bars from the Sloan Digital…

宇宙学与河外天体物理 · 物理学 2015-05-27 Sara L. Ellison , David R. Patton , Preethi Nair , Luc Simard , J. Trevor Mendel , Alan W. McConnachie , Jillian M. Scudder

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

We aim to unravel the interplay between bars, star formation (SF), and active galactic nuclei (AGNs) in barred galaxies. To this end, we utilize the SDSS DR12 to select a sample of nearby (0.02 < z < 0.06) disk galaxies that are suitable…

星系天体物理 · 物理学 2023-06-07 Woong-Bae G. Zee , Sanjaya Paudel , Jun-Sung Moon , Suk-Jin Yoon

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…

Context. Via scaling relations, it is well-known that active galactic nuclei (AGN) and bulges are linked. This link was thought to be driven by mergers, but recent studies show that secular processes are the dominant mechanism of…

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