中文
相关论文

相关论文: Is Centaurus A special? A neutral hydrogen perspec…

200 篇论文

We present new ATCA 21-cm line observations of the neutral hydrogen in the nearby radio galaxy Centaurus A. We image in detail (with a resolution down to 7", ~100pc) the distribution of HI along the dust lane. Our data have better velocity…

宇宙学与河外天体物理 · 物理学 2015-05-18 C. Struve , T. A. Oosterloo , R. Morganti , L. Saripalli

Centaurus A (NGC5128) is a fantastic object, ideal for investigating the characteristics and the role of the gas in an early-type galaxy in the presence of a radio-loud active nucleus. The different phases of the gas - hot (X-ray), warm…

宇宙学与河外天体物理 · 物理学 2015-05-18 Raffaella Morganti

Centaurus A (Cen A) is one of the most famous galaxies hosting an active galactic nucleus (AGN), where the interaction between AGN activities and surrounding interstellar and intergalactic media has been investigated. Recent studies…

星系天体物理 · 物理学 2020-09-17 R. Katayama , H. Kaneda , T. Kokusho , K. Morihana , T. Suzuki , S. Oyabu , M. Yamagishi , T. Tsuchikawa

Centaurus A, at a distance of less than 4 Mpc, is the nearest radio-loud AGN. Its emission is detected from radio to very-high energy gamma-rays. Despite the fact that Cen A is one of the best studied extragalactic objects the origin of its…

高能天体物理现象 · 物理学 2015-05-14 H. Steinle

We present new observations, performed with the Australia Telescope Compact Array, of the HI absorption in the central regions of Centaurus A. For the first time, absorption is detected against the radio core at velocities blueshifted with…

天体物理学 · 物理学 2009-11-13 R. Morganti , T. Oosterloo , C. Struve , L. Saripalli

We present results of an ongoing systematic study of the large-scale properties of neutral hydrogen (HI) gas in nearby radio galaxies. Our main goal is to investigate the importance of gas-rich galaxy mergers and interactions among…

宇宙学与河外天体物理 · 物理学 2009-11-25 Bjorn Emonts , Raffaella Morganti , Christian Struve

We present WSRT and VLA radio observations of the neutral hydrogen in the radio galaxy Coma A. We detect extended HI absorption against both radio lobes of Coma A, at distances of about 30 kpc from the centre. Coma A is the first radio…

天体物理学 · 物理学 2009-11-07 R. Morganti , T. A. Oosterloo , S. Tinti , C. N. Tadhunter , K. A. Wills , G. van Moorsel

We present morphological and statistical results of a study of neutral hydrogen (HI) in a complete sample of nearby, non-cluster radio galaxies. We detect large-scale HI emission in the early-type host galaxies of 25% of our sample sources.…

天体物理学 · 物理学 2008-11-26 B. H. C. Emonts , R. Morganti , T. A. Oosterloo

We present the first results of a study aimed to detect large HI structures in radio galaxies. In two of the three cases presented (Coma A and B2 0648+27), the detection of a large amount of HI distributed over several tens of kpc suggests…

天体物理学 · 物理学 2009-11-07 R. Morganti , T. Oosterloo , C. Tadhunter , B. Emonts

We present new radio and optical images of the nearest radio galaxy Centaurus A and its host galaxy NGC 5128. We focus our investigation on the northern transition region, where energy is transported from the ~5 kpc (~5 arcmin) scales of…

We present Keck II adaptive optics near infrared imaging and spectroscopic observations of the central regions of the powerful radio galaxy Cygnus A. The 0.05" resolution images clearly show an unresolved nucleus between two spectacular…

天体物理学 · 物理学 2009-11-10 Gabriela Canalizo , Claire Max , David Whysong , Robert Antonucci , Scott E. Dahm

For the first time, systematic studies of dwarf galaxies are being conducted throughout the Local Volume, including the dwarf satellites of the nearby giant elliptical galaxy Centaurus A (NGC 5128). Given Centaurus As mass (roughly ten…

星系天体物理 · 物理学 2024-12-04 Sachi Weerasooriya , Mia Sauda Bovill , Matthew A. Taylor , Andrew J. Benson , Cameron Leahy

[abridged] We report on Suzaku observations of selected regions within the Southern giant lobe of the radio galaxy Centaurus A. We focus on distinct X-ray features likely associated with fine radio structure of the lobe. We find that the…

We present first results of new ATCA HI emission and absorption observations of Centaurus A. The large-scale disk is described via a tilted-ring model. A broader redshifted absorption than previously known as well as a blueshifted…

天体物理学 · 物理学 2007-12-13 Christian Struve , Raffaella Morganti , Tom A. Oosterloo

Centaurus A is one of the closest radio-galaxies to Earth. Its proximity allowed us to extensively study its active galactic nucleus but the core emission mechanism remains elusive because of local strong dust and gas obscuration. The…

Neutral atomic hydrogen (HI) observations are fundamental to understand the dynamics of galaxies, their assembly, the fuelling of their star formation and environmental interactions. HI studies have so far been limited by the capabilities…

星系天体物理 · 物理学 2024-08-16 F. M. Maccagni , W. J. G. de Blok

We present new 21-cm HI observations performed with ATCA of the large HI filament located about 15 kpc NE from the centre of Centaurus A and discovered by Schiminovich et al.(1994). This HI cloud is situated (in projection) near the radio…

天体物理学 · 物理学 2009-11-10 T. A. Oosterloo , R. Morganti

This review summarizes the state of the knowledge of the nearby (D = 3.4 Mpc) radio source Centaurus A and its host galaxy NGC 5128. The massive elliptical host galaxy appears to be moderately triaxial. It contains a strongly warped thin…

天体物理学 · 物理学 2009-10-31 F. P. Israel

The study of the optical continuum of radio galaxies shows that about 30% have a young stellar population component. Among them are the most far-IR bright radio galaxies. A further indication of the relatively gas rich environment of these…

天体物理学 · 物理学 2007-05-23 Raffaella Morganti , Tom Oosterloo , Clive Tadhunter , Bjorn Emonts , Gustaaf van Moorsel

We present WSRT observations of the neutral hydrogen in the nearby radio galaxy B2 0648+27. In emission, we detect a very large amount of HI (M_HI = 1.1 x 10^10 M_sun) that is distributed in a very extended disk, or ring-like structure, of…

天体物理学 · 物理学 2009-11-07 R. Morganti , T. A. Oosterloo , A. Capetti , H. R. de Ruiter , R. Fanti , P. Parma , C. N. Tadhunter , K. A. Wills
‹ 上一页 1 2 3 10 下一页 ›