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相关论文: A newly discovered double-double candidate microqu…

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We have studied the newly-discovered microquasar in NGC 7793 in radio, optical and X-ray bands. This system comprises a large (250 x 120 pc) line-emitting optical nebula, detected in H-alpha and HeII 4686. The optical nebula coincides with…

高能天体物理现象 · 物理学 2015-05-14 Roberto Soria , Manfred Pakull , Jess Broderick , Stephane Corbel , Christian Motch

Microquasars are neutron star or black hole X-ray binaries with jets. These jets can create shock-ionized bubbles of hot plasma that can masquerade as peculiar supernova remnants (SNRs) in extragalactic surveys. To see if this is the case…

高能天体物理现象 · 物理学 2020-01-29 Roberto Soria , William P. Blair , Knox S. Long , Thomas D. Russell , P. Frank Winkler

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

We present a multiwavelength examination of the supernova remnant (SNR) S26 in the nearby galaxy NGC 300 using data from Chandra X-ray Observatory, XMM-Newton X-ray Observatory, Hubble Space Telescope (HST), the Very Large Array, and the…

高能天体物理现象 · 物理学 2019-06-12 Jacob Gross , Benjamin F. Williams , Thomas G. Pannuti , Breanna Binder , Kristen Garofali , Zachary G. Hanvey

M33 contains a large number of emission nebulae identified as supernova remnants (SNRs) based on the high [S II]:Ha ratios characteristic of shocked gas. Using Chandra data from the ChASeM33 survey with a 0.35-2 keV sensitivity of about 2 x…

The X-ray binary SS 433, embedded in the W50 nebula (or supernova remnant W50), shows bipolar jets that are ejected with mildly relativistic velocities, and extend toward the east and west out to scales of tens of parsecs. Previous X-ray…

We present a broadband X-ray study of W50 (`the Manatee nebula'), the complex region powered by the microquasar SS 433, that provides a test-bed for several important astrophysical processes. The W50 nebula, a Galactic PeVatron candidate,…

We have made a 30 ksec Chandra observation of the redshift z=0.63 GPS quasar B2 0738+313. We detected X-ray emission from the core and have discovered a 200 kpc (projected on the sky) X-ray jet. The X-ray jet is narrow and curves, following…

We report XMM-Newton observations of the Galactic supernova remnant G296.8-0.3, together with complementary radio and infrared data. The spatial and spectral properties of the X-ray emission, detected towards G296.8-0.3, was investigated in…

高能天体物理现象 · 物理学 2015-05-30 E. Sánchez-Ayaso , J. A. Combi , J. F. Albacete Colombo , J. López-Santiago , J. Martí , A. J. Muñoz-Arjonilla

We present results from {\em Chandra}/ACIS-S, {\em Spitzer}, {\em XMM-Newton}, {\em HST}, and VLA observations of the radio hot spots, extended environment, and nucleus of the nearby ($z$=0.0597) FR II radio galaxy 3C 33. This is a…

天体物理学 · 物理学 2011-02-11 R. P. Kraft , M. Birkinshaw , M. J. Hardcastle , D. A. Evans , J. H. Croston , D. M. Worrall , S. S. Murray

We recently reported the discovery of a candidate jet-driving microquasar (S10) in the nearby spiral galaxy NGC 300. However, in the absence of kinematic information, we could not reliably determine the jet power or the dynamical age of the…

We report on the discovery of a pointlike source (CXOU J160103.1$-$513353) at the center of a Galactic supernova remnant (SNR) G330.2+1.0 with {\it Chandra X-Ray Observatory}. The X-ray spectrum fits a black-body (BB) model with $kT$ $\sim$…

We report the detection at X-rays of the radio/optical hotspot and knots of 3C 303 from a short (15 ksec) Chandra exposure in 2001 March. The X-ray morphology is similar to that of the radio/optical emission with peaks in the X-ray emission…

天体物理学 · 物理学 2009-11-07 Jun Kataoka , Philip Edwards , Markos Georganopoulos , Fumio Takahara , Stefan Wagner

Very Large Telescope adaptive optics images of NGC 253 with resolutions down to 200 mas resolve the central 300 pc of this galaxy in ~ 37 infrared (IR) bright knots, a factor of 3 larger than previously reported, and extended diffuse…

The supernova remnant (SNR) W51C is a Galactic object located in a strongly inhomogeneous interstellar medium with signs of an interaction of the SNR blast wave with dense molecular gas. Diffuse X-ray emission from the interior of the SNR…

高能天体物理现象 · 物理学 2014-03-05 Manami Sasaki , Cornelia Heinitz , Gabriele Warth , Gerd Puehlhofer

Aims: We study the supernova remnant G20.0-0.2 and its surroundings in order to look for the high energy counterpart of the radio nebula and to find evidence of interaction between the shock front and the interstellar medium. Methods: We…

星系天体物理 · 物理学 2015-06-15 Alberto Petriella , Sergio Paron , Elsa Giacani

Context: HH 158, the jet from the young star DG Tau, is one of the few sources of its type where jet knots have been detected at optical and X-ray wavelengths. Aims: To search, using Very Large Array observations of this source, radio knots…

星系天体物理 · 物理学 2015-06-03 L. F. Rodriguez , R. F. Gonzalez , A. C. Raga , J. Canto , A. Riera , L. Loinard , S. A. Dzib , L. A. Zapata

We present a combined radio, optical, and X-ray study of the nearby LINER galaxy NGC 1052. Data from a short (2.3 ksec) {\it CHANDRA} observation of NGC 1052 reveal the presence of various jet-related X-ray emitting regions, a bright…

天体物理学 · 物理学 2009-11-10 M. Kadler , J. Kerp , E. Ros , H. Falcke , R. W. Pogge , J. A. Zensus

We report Chandra imaging-spectroscopy and RXTE spectroscopy of the nearby, powerful radio galaxy Cygnus A. Various aspects of the results are discussed, including the X-ray properties of the nucleus, the radio hot spots, the cluster of…

天体物理学 · 物理学 2007-05-23 A. S. Wilson , K. A. Arnaud , D. A. Smith , Y. Terashima , A. J. Young

We have studied the structure and energetics of the powerful microquasar/shock-ionized nebula S26 in NGC 7793, with particular focus on its radio and X-ray properties. Using the Australia Telescope Compact Array, we have resolved for the…

高能天体物理现象 · 物理学 2015-05-19 Roberto Soria , Manfred W. Pakull , Jess W. Broderick , Stephane Corbel , Christian Motch
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