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相关论文: A Radio Nebula Surrounding the Ultra-luminous X-ra…

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In this letter, we report on dual-frequency European VLBI Network (EVN) observations of the faintest and least luminous radio cores in Seyfert nuclei, going to sub-mJy flux densities and radio luminosities around 10^19 W/Hz. We detect radio…

宇宙学与河外天体物理 · 物理学 2014-11-20 Marcello Giroletti , Francesca Panessa

The AGN NGC 2110 presents a peculiar case among the Seyfert 2 galaxies, as it displays also features of radio-loud objects and is classified as FR-I radio galaxy. Here we analyse simultaneous INTEGRAL and Swift data taken in 2008 and 2009.…

宇宙学与河外天体物理 · 物理学 2011-02-28 Volker Beckmann , Olivier Do Cao

We report the spectral analysis of a long XMM-Newton observation of the well-studied, moderate luminosity Broad Line Seyfert 1 galaxy NGC 5548. The source was at an historically average brightness and we find the hard (3-10 keV) spectrum…

天体物理学 · 物理学 2011-07-19 K. A. Pounds , J. N. Reeves , K. L. Page , R. Edelson , G. Matt , G. C. Perola

PKS 0558-504 is the brightest radio-loud Narrow-Line Seyfert 1 galaxy at X-ray energies. Here we present results from the radio, optical, UV, and X-ray bands obtained with Swift, XMM, and ATCA during a 10-day monitoring campaign in…

高能天体物理现象 · 物理学 2015-05-19 M. Gliozzi , I. E. Papadakis , D. Grupe , W. P. Brinkmann , C. Raeth , L. Kedziora-Chudczer

In a search for low surface brightness radio nebulae using the ASKAP-EMU survey, we discovered a faint radio shell, G289.6+5.8, and its central point radio source at the position of the soft gamma-ray source IGR J11187-5438. The central…

Combining Chandra, ALMA, EVLA, and Hubble Space Telescope archival data and newly acquired APO/DIS spectroscopy, we detect a double-lobed 17~kpc X-ray emission with plumes oriented approximately perpendicular and parallel to the galactic…

We report on a powerful and variable off-nuclear X-ray source in the nearby spiral galaxy NGC 4945. Two ROSAT PSPC observations show the source to brighten in 0.5--2.0 keV flux by a factor of about 9 on a time-scale of 11 months or less. It…

天体物理学 · 物理学 2016-06-08 W. N. Brandt , K. Iwasawa , C. S. Reynolds

We present deep GALEX images of NGC 5128, the parent galaxy of Centaurus A. We detect a striking "weather ribbon" of Far-UV and H$\alpha$ emission, which extends more than 35 kpc northeast of the galaxy. The ribbon is associated with a…

星系天体物理 · 物理学 2015-06-23 Susan G. Neff , Jean A. Eilek , Frazer N. Owen

We present a deep optical imaging campaign on the starburst galaxy NGC 4631 with CFHT/MegaCam. By supplementing the HST/ACS and Chandra/ACIS archival data, we search for the optical counterpart candidates of the five brightest X-ray sources…

We present the first Chandra detection of a single X-ray cavity within the interstellar medium of the small Fanaroff-Riley type I (FRI) radio galaxy NGC 5141. The X-ray surface brightness depression, located $\approx 4$ kpc away from the…

星系天体物理 · 物理学 2022-04-20 Duccio Macconi , Paola Grandi , Myriam Gitti , Cristian Vignali , Eleonora Torresi , Fabrizio Brighenti

We present radio continuum observations of NGC 2082 using ASKAP, ATCA and Parkes telescopes from 888 MHz to 9000 MHz. Some 20 arcsec from the centre of this nearby spiral galaxy, we discovered a bright and compact radio source,…

星系天体物理 · 物理学 2022-07-05 Joel C. F. Balzan , Miroslav D. Filipovic , Shi Dai , Rami Z. E. Alsaberi , Luke Barnes

We present Chandra observations of two relatively high redshift FRII radio galaxies, 3C 432 and 3C 191 (z=1.785 and z=1.956 respectively), both of which show extended X-ray emission along the axis of the radio jet or lobe. This X-ray…

天体物理学 · 物理学 2009-09-17 M. C. Erlund , A. C. Fabian , Katherine M. Blundell , A. Celotti , C. S. Crawford

We aim to determine the properties of the central region of NGC 1052 using X-ray and radio data. NGC 1052 (z=0.005) has been investigated for decades in different energy bands and shows radio lobes and a low luminosity active galactic…

星系天体物理 · 物理学 2020-07-01 S. Falocco , J. Larsson , S. Nandi

We have combined Hubble Space Telescope/Faint Object Spectrograph, ground-based, and Infrared Space Observatory spectra of the nucleus of NGC 4395, the least luminous and nearest known type 1 Seyfert galaxy. The spectra show emission lines…

We present the first X-ray observation at sub-arcsecond resolution of the high-redshift ($z=6.18$) radio-loud quasar CFHQS J142952+544717 (J1429). The ~100 net-count 0.3-7 keV spectrum obtained from $\sim 30$ ksec Chandra exposure is best…

高能天体物理现象 · 物理学 2023-07-12 G. Migliori , A. Siemiginowska , M. Sobolewska , C. C. Cheung , Ł. Stawarz , D. Schwartz , B. Snios , A. Saxena , V. Kashyap

We report the VLA detection of the radio counterpart of the X-ray object referred to as the "Cannonball", which has been proposed to be the remnant neutron star resulting from the creation of the Galactic Center supernova remnant,…

高能天体物理现象 · 物理学 2015-06-17 Jun-Hui Zhao , Mark R. Morris , W. M. Goss

We report the discovery of a flaring X-ray source in the globular cluster NGC 6540, obtained during the EXTraS project devoted to a systematic search for variability in archival data of the XMM-Newton satellite. The source had a quiescent…

The results of a 0.4-10.0 keV ASCA spectral analysis of a sample of low-luminosity AGN (LLAGN; M51, NGC 3147, NGC 4258), low-ionization nuclear emission line regions (LINERs; NGC 3079, NGC 3310, NGC 3998, NGC 4579, NGC 4594) and starburst…

天体物理学 · 物理学 2009-10-30 A. Ptak , P. Serlemitsos , T. Yaqoob , R. Mushotzky

During the course of an investigation of the interaction of the radio galaxy M84 and its ambient cluster gas, we found excess X-ray emission aligned with the northern radio jet. The emission extends from the X-ray core of the host galaxy as…

天体物理学 · 物理学 2009-11-07 D. E. Harris , A. Finoguenov , A. H. Bridle , M. J. Hardcastle , R. A. Laing

The first short Chandra and XMM-Newton observations of the young and energetic pulsar J1357-6429 provided strong indications of a tail-like pulsar-wind nebula associated with this object, as well as pulsations of its X-ray flux with a…

天体物理学 · 物理学 2009-11-13 Vyacheslav E. Zavlin