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相关论文: Dense gas without star formation: The kpc-sized mo…

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We present a detailed analysis of the gas conditions in the H_2 luminous radio galaxy 3C326N at z~0.1, which has a low star formation rate (SFR~0.07 M_sun/yr) in spite of a gas surface density similar to those in starburst galaxies. Its…

宇宙学与河外天体物理 · 物理学 2015-05-18 N. P. H. Nesvadba , F. Boulanger , P. Salome , P. Guillard , M. D. Lehnert , P. Ogle , P. Appleton , E. Falgarone , G. Pineau des Forets

The physical link between AGN activity and the suppression of star formation in their host galaxies is one of the major open questions of AGN feedback. The Spitzer space mission revealed a subset of nearby radio galaxies with unusually…

We detect bright [CII]158$\mu$m line emission from the radio galaxy 3C 326N at z=0.09, which shows weak star formation ($SFR<0.07$M$_{\odot}$~yr$^{-1}$) despite having strong H$_2$ line emission and $2\times 10^9$M$_{\odot}$ of molecular…

星系天体物理 · 物理学 2015-01-21 P. Guillard , F. Boulanger , M. D. Lehnert , G. Pineau des Forêts , F. Combes , E. Falgarone , J. Bernard-Salas

How efficiently star formation proceeds in galaxies is still an open question. Recent studies suggest that AGN can regulate the gas accretion and thus slow down star formation (negative feedback). However, evidence of AGN positive feedback…

星系天体物理 · 物理学 2015-01-21 Q. Salomé , P. Salomé , F. Combes

We use JWST/NIRSpec observations of the radio galaxy 3C 293 to map the emission, extinction, and kinematics of hot molecular and ionized gas, as well as stellar kinematics, within the inner ~ 2 kpc. The stellar velocity field is well…

Aims. We investigate the different manifestations of AGN feedback in the evolved, powerful radio source 3C293 and their impact on the molecular gas of its host galaxy, which harbors young star-forming regions and fast outflows of HI and…

星系天体物理 · 物理学 2014-05-08 A. Labiano , S. Garcia-Burillo , F. Combes , A. Usero , R. Soria-Ruiz , J. Piqueras Lopez , A. Fuente. , L. Hunt , R Neri

The radio galaxy 3C 273 hosts one of the nearest and best-studied powerful quasar jets. Having been imaged repeatedly by the Hubble Space Telescope (HST) over the past twenty years, it was chosen for an HST program to measure proper motions…

We present millimeter molecular-line complemented by optical observations, along with a reanalysis of archival centimeter HI and continuum data, to infer the global dynamics and determine where dense molecular gas and massive stars…

星系天体物理 · 物理学 2015-06-15 Hsi-An Pan , Jeremy Lim , Satoki Matsushita , Tony Wong , Stuart Ryder

Aims: We study the emission of molecular gas in 3C236, a FR II radio source at z~0.1, and search for the footprints of AGN feedback. 3C236 shows signs of a reactivation of its AGN triggered by a recent minor merger episode. Observations…

宇宙学与河外天体物理 · 物理学 2015-06-11 A. Labiano , S. Garcia-Burillo , F. Combes , A. Usero , R. Soria-Ruiz , G. Tremblay , R. Neri , A. Fuente , R. Morganti , T. Oosterloo

Gas and dust in star-forming galaxies at the peak epoch of galaxy assembly are presently the topic of intense study, but little is known about the interstellar medium (ISM) of distant, passively evolving galaxies. We report on a deep 3…

星系天体物理 · 物理学 2015-06-17 Mark T. Sargent , E. Daddi , F. Bournaud , M. Onodera , C. Feruglio , M. Martig , R. Gobat , H. Dannerbauer , E. Schinnerer

We present the results of large-area CO J=3-2 emission mapping of three nearby field galaxies, NGC 628, NGC 3521, and NGC 3627, completed at the James Clerk Maxwell Telescope as part of the Nearby Galaxies Legacy Survey. These galaxies all…

We study the interactions of a relativistic jet with a dense turbulent gaseous disk of radius $\sim 2$ kpc. We have performed a suite of simulations with different mean density, jet power and orientation. Our results show that: A) the…

高能天体物理现象 · 物理学 2018-07-18 Dipanjan Mukherjee , Geoffrey V. Bicknell , Alexander Y. Wagner , Ralph S. Sutherland , Joseph Silk

We report the discovery of shocked molecular and ionized gas resulting from jet-driven feedback in the compact radio galaxy 4C 31.04 using near-IR imaging spectroscopy. 4C 31.04 is a $\sim 100$ pc double-lobed Compact Steep Spectrum source…

We report the detection of outflowing molecular gas at the center of the nearby radio galaxy NGC6328 (z=0.014), which has a gigahertz-peaked spectrum radio core and a compact (2 pc) young double radio lobe tracing jet. Utilizing Atacama…

Galactic disks consist of both stars and gas. The gas is more dynamically responsive than the stars, and strongly nonlinear structures and velocities can develop in the ISM even while stellar surface density perturbations remain…

天体物理学 · 物理学 2011-02-11 Woong-Tae Kim , Eve C. Ostriker

Querying the Spitzer archive for optically-selected active galactic nuclei (AGN) observed in high-resolution mode spectroscopy, we identified radio and/or interacting galaxies with highly turbulent motions of the H2 gas at a temperature of…

宇宙学与河外天体物理 · 物理学 2011-10-19 K. M. Dasyra , F. Combes

We present an unprecedented view on the morphology and kinematics of the extended narrow-line region (ENLR) and molecular gas around the prototypical hyper-luminous quasar 3C273 ($L\sim10^{47}$ erg/s at z=0.158) based on VLT-MUSE optical 3D…

星系天体物理 · 物理学 2019-07-17 B. Husemann , V. N. Bennert , K. Jahnke , T. A. Davis , J. -H. Woo , J. Scharwächter , A. Schulze , M. Gaspari , M. Zwaan

We analyse the 2-dimensional distribution and kinematics of the stars as well as molecular and ionised gas in the central few hundred parsecs of 5 active and 5 matched inactive galaxies. The equivalent widths of the Br-gamma line indicate…

We discuss the dense molecular gas in central regions of nearby Seyfert galaxies, and report new arcsec resolution observations of HCN(1-0) and HCO$^+$(1-0) for 3 objects. In NGC 3079 the lines show complex profiles as a result of…

We present results from a study of the dense circum-nuclear molecular gas of starburst galaxies. The study aims to investigate the interplay between starbursts, active galactic nuclei and molecular gas. We characterise the dense gas traced…

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