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相关论文: Formation of Ionization-Cone Structures in Active …

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There are few observational constraints on how the escape of ionizing photons from starburst galaxies depends on galactic parameters. Here, we report on the first major detection of an ionization cone in NGC 5253, a nearby starburst galaxy.…

宇宙学与河外天体物理 · 物理学 2015-05-30 Jordan Zastrow , M. S. Oey , Sylvain Veilleux , Michael McDonald , Crystal L. Martin

We consider the propagation and stability of the helical electromagnetic perturbations in a relativistic force-free Pointing flux dominated jet (magnetic helix). Perturbations are found to dissipate energy in the vicinity of the resonant…

天体物理学 · 物理学 2007-05-23 V. I. Pariev , Ya. N. Istomin , A. R. Beresnyak

The recently identified Circinus Galaxy is the nearest (about 4 Mpc) Seyfert 2 galaxy known and we now demonstrate to be one of the best laboratories for studying the effects of nuclear activity on the surrounding environment. Here we…

天体物理学 · 物理学 2009-10-30 S. Veilleux , J. Bland-Hawthorn

We present an analysis of the X-ray spectra of a sample of 37 observations of 26 Seyfert galaxies observed by XMM-Newton in order to characterize their iron K emission. All objects show evidence for iron line emission in the 6-7 keV band. A…

天体物理学 · 物理学 2009-11-13 K. Nandra , P. M. O'Neill , I. M. George , J. N. Reeves

A sample of the brightest known Seyfert galaxies from the CfA sample is analyzed on the basis of ISO photometric and spectroscopic data. Regardless of the Seyfert type, the mid-IR continuum emission from these galaxies is found to be…

天体物理学 · 物理学 2016-08-30 M. Almudena Prieto , A. M. Perez Garcia , J. M. Rodriguez Espinosa

We present sub-arcsec near-infrared 1.5 - 2.5 micron moderate resolution long-slit spectra of eight nearby Seyfert galaxies (z<0.01), both parallel to the ionization cone and perpendicular to it. These spectra complement similar data on six…

天体物理学 · 物理学 2009-11-07 J. Reunanen , J. Kotilainen , M. A. Prieto

The narrow emission line spectra of active galactic nuclei are not accurately described by simple photoionization models of single clouds. Recent Hubble Space Telescope images of Seyfert 2 galaxies show that these objects are rich with…

天体物理学 · 物理学 2009-10-30 Jason W. Ferguson , Kirk T. Korista , Jack A. Baldwin , Gary J. Ferland

A number of radio galaxies has been detected by Fermi/LAT in the gamma-ray domain. In some cases, like Cen A and M 87, these objects have been seen even in the TeV range by Cherenkov telescopes. Whereas the gamma-ray emission is likely to…

高能天体物理现象 · 物理学 2013-02-20 V. Beckmann , S. de Jong , F. Mattana , D. Saez , S. Soldi

We investigate the correlation between ionized gas outflows, jets, and star formation in a sample of 42 local type-I active galactic nuclei (AGNs) exhibiting significant [O III] outflows. This study uses both new submillimeter (sub-mm)…

星系天体物理 · 物理学 2026-01-16 Chen Qin , Huynh Anh N. Le , Yongquan Xue , Shifu Zhu , Xiaozhi Lin , Kim Ngan Nhat Nguyen

Recent {\it ASCA} observations confirm the presence of X-ray absorption due to partially ionized gas in many Seyfert 1 galaxies; the so-called warm absorber. Constraints on the location of the warm material are presented with the conclusion…

天体物理学 · 物理学 2015-06-24 C. S. Reynolds , A. C. Fabian

We present the detection of compact radio structures of fourteen radio-loud narrow line Seyfert 1 (NLS1) galaxies from Very Long Baseline Array observations at 5 GHz, which were performed in 2013. While 50\% of the sources of our sample…

星系天体物理 · 物理学 2015-10-14 Minfeng Gu , Yongjun Chen , S. Komossa , Weimin Yuan , Zhi-Qiang Shen , Kiyoaki Wajima , Hongyan Zhou , J. A. Zensus

In this paper we explore collisional ionization and time-evolving photoionization in the, X-ray discovered, ionized absorbers in Seyfert galaxies. These absorbers show temporal changes inconsistent with simple equilibrium models. We develop…

天体物理学 · 物理学 2009-10-30 F. Nicastro , F. Fiore , G. C. Perola , M. Elvis

Massive stars influence their parental molecular cloud, and it has long been suspected that the development of hydrodynamical instabilities can compress or fragment the cloud. Identifying such instabilities has proved difficult. It has been…

星系天体物理 · 物理学 2010-11-02 Olivier Berné , Núria Marcelino , José Cernicharo

Neumayer et al. established the existence of a blue-shifted cloud in the core of Centaurus A, within a few parsecs of the nucleus and close to the radio jet. We propose that the cloud has been impacted by the jet, and that it is in the…

高能天体物理现象 · 物理学 2015-06-15 Geoffrey V. Bicknell , Ralph S. Sutherland , Nadine Neumayer

The launch of the Infrared Space Observatory and new atomic data have opened a window to the study of high ionization gas in active galactic nuclei (AGN). We present the results of a large number of photoionization simulations of the…

天体物理学 · 物理学 2009-10-30 Jason W. Ferguson , Kirk T. Korista , Gary J. Ferland

We have observed a sample of 157 Seyfert galaxies with a 275 km baseline radio interferometer to search for compact, high brightness temperature radio emission from the active nucleus. We obtain the surprising result that compact radio…

天体物理学 · 物理学 2009-10-22 A. L. Roy , R. P. Norris , M. J. Kesteven , E. R. Troup , J. E. Reynolds

In recent years it has become increasingly clear that Active Galactic Nuclei, and radio-galaxies in particular, have an impact on large scale structure and galaxy formation. In principle, radio-galaxies are energetic enough to halt the…

天体物理学 · 物理学 2009-11-13 John C. Vernaleo , Christopher S. Reynolds

Seyfert galaxies commonly host compact jets spanning 10-100 pc scales, but larger structures (KSRs) are resolved out in long baseline, aperture synthesis surveys. We report a new, short baseline Very Large Array (VLA) survey of a complete…

天体物理学 · 物理学 2008-11-26 J. F. Gallimore , D. J. Axon , C. P. O'Dea , S. A. Baum , A. Pedlar

New observations using narrow band imaging, long-slit spectroscopy and MERLIN observations of the nuclear region of the Seyfert galaxy NGC~4051 have been made. An edge brightened, triangular region of ionized gas extending 420 pc from the…

We investigate the spatially-resolved star formation relation using a galactic disk formed in a comprehensive high-resolution (3.8 pc) simulation. Our new implementation of stellar feedback includes ionizing radiation as well as supernova…

星系天体物理 · 物理学 2018-03-12 Ji-hoon Kim , Mark R. Krumholz , John H. Wise , Matthew J. Turk , Nathan J. Goldbaum , Tom Abel