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相关论文: Sub-parsec scale imaging of Centaurus A

200 篇论文

Centaurus B is a nearby radio galaxy positioned in the Southern hemisphere close to the Galactic plane. Here we present a detailed analysis of about 43 months of accumulated Fermi-LAT data of the gamma-ray counterpart of the source…

高能天体物理现象 · 物理学 2015-06-12 J. Katsuta , Y. T. Tanaka , L. Stawarz , S. P. O'Sullivan , C. C. Cheung , J. Kataoka , S. Funk , T. Yuasa , H. Odaka , T. Takahashi , J. Svoboda

We have performed a very long baseline interferometry (VLBI) survey of local (z < 0.05) ultra hard X-ray (14-195 keV) selected active galactic nuclei (AGN) from the Swift Burst Alert Telescope (BAT) using KVN, KaVA, and VLBA. We first…

A 45 deg2 radio continuum imaging campaign of the nearest radio galaxy, Centaurus A, is reported. Using the Australia Telescope Compact Array and the Parkes 64m radio telescope at 1.4 GHz, the spatial resolution of the resultant image is…

We present high angular resolution X-ray images and spectra from two {\em Chandra} ACIS-I observations of the X-ray jet in the nearby radio galaxy Centaurus A. We find that the X-ray emission from the jet is composed of a low surface…

天体物理学 · 物理学 2009-11-07 R. P. Kraft , W. R. Forman , C. Jones , S. S. Murray , M. J. Hardcastle , D. M. Worrall

Centaurus A (Cen A) is the nearest radio-loud AGN and is detected from radio to very high energy gamma-rays. Its nuclear spectral energy distribution (SED) shows a double-peak feature, which is well explained by the leptonic synchrotron +…

高能天体物理现象 · 物理学 2015-06-03 Sarira Sahu , Bing Zhang , Nissim Fraija

We present results from the Very Long Baseline Array (VLBA) multi-frequency (1.6, 4.4, 8.6, 22 GHz), high-sensitivity (~25 microJy beam^-1), sub-parsec scale (<1 pc) observations and Spectral Energy Distributions (SEDs) for a sample of 12…

Ever since the discovery by the Fermi mission that active galactic nuclei (AGN) produce copious amounts of high-energy emission, its origin has remained elusive. Using high-frequency radio interferometry (VLBI) polarization imaging, we…

高能天体物理现象 · 物理学 2018-05-15 B. Rani , S. G. Jorstad , A. P. Marscher

The TANAMI (Tracking AGN with Austral Milliarcsecond Interferometry) program provides comprehensive VLBI monitoring of extragalactic gamma-ray sources south of declination -30 degrees. Operating at two radio frequencies (8 and 22 GHz), this…

宇宙学与河外天体物理 · 物理学 2010-06-11 Roopesh Ojha , Matthias Kadler , Moritz Boeck , Faith Hungwe , Cornelia Mueller , Joern Wilms , Eduardo Ros , the TANAMI Team

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…

We recently announced the detection of an unknown submillimeter source in our ALMA observations of alpha Cen AB. The source was detected in two epochs, a strong detection at 445~GHz and one at lower significance at 343.5~GHz. After valuable…

太阳与恒星天体物理 · 物理学 2015-12-18 R. Liseau , W. Vlemmings , E. O'Gorman , E. Bertone , M. Chavez , V. De la Luz

We present results from a sensitive high-resolution X-ray observation of the nearby active galaxy Centaurus A (NGC 5128) with the ROSAT HRI. The 65~ksec X-ray image clearly distinguishes different components of the X-ray emission from Cen…

天体物理学 · 物理学 2009-10-28 S. Doebereiner , N. Junkes , S. J. Wagner , H. Zinnecker , R. Fosbury , G. Fabbiano , E. J. Schreier

As the closest known active galactic nucleus, Centaurus A (Cen A) provides a rich environment for astrophysical exploration. It has been observed across wavelengths from radio to gamma rays, and indications of ongoing particle acceleration…

高能天体物理现象 · 物理学 2025-04-04 Cainã de Oliveira , James H. Matthews , Vitor de Souza

As the closest radio galaxy, Centaurus A is a powerful laboratory for the X-ray study of radio-emitting structures and their interactions with the hot interstellar medium (ISM). This paper details our interpretation of the remarkable X-ray…

天体物理学 · 物理学 2007-05-23 D. M. Worrall , R. P. Kraft , M. Birkinshaw , M. J. Hardcastle , W. R. Forman , C. Jones , S. S. Murray

The {\gamma}-ray data of Fermi-LAT on the giant lobes of Centaurus A are analysed together with the high frequency radio data obtained with the Planck satellite. The large {\gamma}-ray photon statistics, accumulated during seven years of…

高能天体物理现象 · 物理学 2017-08-09 Xiao-na Sun , Rui-zhi Yang , Benjamin Mckinley , Felix Aharonian

We present high spatial resolution mid-IR images of the nuclear region of NGC 5128 (Centaurus A). Images were obtained at 8.8 micron, N-band (10.4 micron), and 18.3 micron using the mid-IR imager/spectrometer T-ReCS on Gemini South. These…

EGRET has detected 67 sources associated with active galactic nuclei. With the exception of radio galaxy Cen A, all are classified as belonging to the blazar class of active galactic nuclei. The cumulative exposure from multiple EGRET…

天体物理学 · 物理学 2010-12-03 P. Sreekumar , D. L. Bertsch , R. C. Hartman , P. L. Nolan , D. J. Thompson

We present X-ray spectra of the nucleus of the nearby radio galaxy Centaurus A from observations with the XMM-Newton EPIC CCD cameras (two exposures separated by 12 months) and the Chandra HETGS. For the first time in an FRI type galaxy, we…

天体物理学 · 物理学 2007-05-23 D. A. Evans , R. P. Kraft , D. M. Worrall , M. J. Hardcastle , C. Jones , W. R. Forman , S. S. Murray

Radio and gamma-ray emission from active galactic nuclei (AGN) are thought to share a common origin, related to the ejection phenomena in the vicinity of supermassive black holes. Thanks to its sensitivity, surveying capability, and broad…

宇宙学与河外天体物理 · 物理学 2010-01-29 M. Giroletti , A. Reimer , L. Fuhrmann , V. Pavlidou , J. L. Richards

The nearby radio galaxy Centaurus A is poorly studied at high frequencies with conventional radio telescopes because of its very large angular size, but is one of a very few extragalactic objects to be detected and resolved by the Wilkinson…

天体物理学 · 物理学 2009-11-13 M. J. Hardcastle , C. C. Cheung , I. J. Feain , L. Stawarz

The interaction between the radio plasma ejected by the active nucleus of a galaxy and the surrounding medium is a key process that can have a strong impact on the interstellar medium of the galaxy and hence on galaxy evolution. The closest…

星系天体物理 · 物理学 2015-11-10 F. Santoro , J. B. R. Oonk , R. Morganti , T. Oosterloo