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相关论文: The Cygnus X region XXIII. Is 18P87 galactic or ex…

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A number of extragalactic radio sources which exhibit symmetric jets on parsec scales have now been found to have neutral hydrogen absorption at or near the systemic velocities of their host galaxies. Understanding the spatial distribution…

天体物理学 · 物理学 2009-11-06 A. B. Peck , G. B. Taylor

The ultra--high energy cosmic rays recently detected by several air shower experiments could have an extragalactic origin. In this case, the nearest active galaxy Centaurus A might be the source of the most energetic particles ever detected…

广义相对论与量子宇宙学 · 物理学 2011-05-23 G. E. Romero , J. A. Combi , S. E. Perez Bergliaffa , L. A. Anchordoqui

Aims: Probe the high-energy ($>$60 MeV) emission from the black hole X-ray binary system, Cygnus X-1, and investigate its origin. Methods: We analysed 7.5 yr of data by Fermi/LAT with the latest PASS8 software version. Results: We report…

We report new radio imaging of the large scale radio structure of M87 with the VLA at 90 cm. These new images show the complex structure of the radio emission more clearly than previous attempts, some of which date back to the 1940's. The…

天体物理学 · 物理学 2009-10-31 F. N. Owen , J. a Eilek , N. E. Kassim

Context. The microquasar 1E 1740.7-2942 is a source located in the direction of the Galactic Center. It has been detected at X-rays, soft gamma-rays, and in the radio band, showing an extended radio component in the form of a double-sided…

天体物理学 · 物理学 2009-11-11 V. Bosch-Ramon , G. E. Romero , J. M. Paredes , A. Bazzano , M. Del Santo , L. Bassani

Cygnus X-3 is a high-mass X-ray binary with a compact object accreting matter from a Wolf-Rayet donor star. Recently, it has been revealed by the Imaging X-ray Polarimetry Explorer (IXPE) as a hidden Galactic ultra-luminous X-ray (ULX)…

We report on the filament of ionized gas found at the NE periphery of M87, the second brightest elliptical galaxy in the Virgo cluster. The object lies at 3.16 arcmin (15.7 kpc) projected distance of the nucleus of M87, and it coincides in…

天体物理学 · 物理学 2007-05-23 G. Gavazzi , A. Boselli , J. M. Vilchez , J. Iglesias-Paramo , C. Bonfanti

A new class of X-ray sources was clearly established with the discovery of highly relativistic radio jets from the galactic sources GRS 1915+105 and GRO J1655-40. Both of these objects have given us a broader view of black holes and the…

天体物理学 · 物理学 2007-05-23 B. A. Harmon

As a prerequisite for interpreting new observations of the most distant radio galaxies, we make an optical study of the closest powerful radio source, Cygnus A. Using Keck imaging- and spectro-polarimetry in conjunction with HST, WFPC2…

天体物理学 · 物理学 2007-05-23 R. A. E. Fosbury , J. Vernet , M. Villar-Martin , M. H. Cohen , P. M. Ogle , H. D. Tran , R. N. Hook

The possible origin of millisecond bursts from the giant elliptical galaxy M87 has been scrutinized since the earliest searches for extragalactic fast radio transients undertaken in the late 1970s. Motivated by rapid technological…

高能天体物理现象 · 物理学 2021-10-13 Akshay Suresh , Shami Chatterjee , James M. Cordes , Fronefield Crawford

We aim at clarifying the nature of the emission of two spatially related unidentified X-ray sources detected with XMM-Newton telescope at intermediate-low Galactic latitude. Observations reveal a point-like source aligned with elongated…

高能天体物理现象 · 物理学 2015-11-25 Federico García , Jorge A. Combi , María C. Medina , Gustavo E. Romero

The radio sky is poorly sampled for rapidly varying transients because of the narrow field-of-view of most imaging radio telescopes at cm and shorter wavelengths. The emergence of sensitive long wavelength observations with intrinsically…

We report the first detection of radio emission from any anomalous X-ray pulsar (AXP). Data from the Very Large Array (VLA) MAGPIS survey with angular resolution 6" reveals a point-source of flux density 4.5 +/- 0.5 mJy at 1.4 GHz at the…

天体物理学 · 物理学 2009-11-13 J. P. Halpern , E. V. Gotthelf , R. H. Becker , D. J. Helfand , R. L. White

We report the detection of fast (~ 1000 km/s), massive outflows of neutral gas observed -- using the WSRT -- as 21-cm HI absorption against the strong radio continuum of seven radio sources. The neutral outflows occur, in at least somes…

天体物理学 · 物理学 2009-11-11 R. Morganti , C. N. Tadhunter , T. A. Oosterloo

We present a 200 ks Chandra ACIS-I image of Cygnus A, and discuss a long linear feature seen in its counterlobe. This feature has a non-thermal spectrum and lies on the line connecting the brighter hotspot on the approaching side and the…

天体物理学 · 物理学 2009-06-23 K. C. Steenbrugge , K. M. Blundell , P. Duffy

We present multi-frequency radio continuum as well as HI observations of the composite galaxy NGC6764, which has a young, circumnuclear starburst and also harbours an active galactic nucleus (AGN). These observations have been made at a…

天体物理学 · 物理学 2009-11-11 Ananda Hota , D. J. Saikia

Massive outflows of neutral atomic hydrogen (HI) have been observed in absorption in a number of radio galaxies and are considered a signature of AGN feedback. These outflows on kpc-scales have not been investigated in great detail as they…

星系天体物理 · 物理学 2021-03-17 R. Schulz , R. Morganti , K. Nyland , Z. Paragi , E. K. Mahony , T. Oosterloo

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

Twenty-two powerful radio galaxies have been searched for HI absorption. We find the highest probability of detecting HI in absorption among narrow-line compact (or small) galaxies or galaxies with indication of richer interstellar medium…

天体物理学 · 物理学 2007-05-23 R. Morganti , T. A. Oosterloo , G. van Moorsel , C. N. Tadhunter , N. Killeen