中文
相关论文

相关论文: 4C 39.29 - extended emission around a powerful Typ…

200 篇论文

We have observed the Orion Molecular Clouds 2 and 3 (OMC-2 and OMC-3) with the Chandra X-ray Observatory (CXO). The northern part of OMC-3 is found to be particularly rich in new X-ray features; four hard X-ray sources are located in and…

The sources discovered in deep hard X-ray surveys with 2-8 keV fluxes of 10^-14 erg cm^-2 s^-1 make up the bulk of the X-ray background at these energies. We present here detailed multi-wavelength observations of three such sources from the…

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 present the results of an HST and ground-based imaging study of a complete 3C sample of z ~ 1 sources, including 5 quasars and 5 radio galaxies. We have resolved continuum structure around all of our quasars in the WFPC2 images and in…

天体物理学 · 物理学 2009-10-30 Susan E. Ridgway , Alan Stockton

Our 5 ks Chandra ACIS-S observation of the globular cluster NGC 6652 detected 7 X-ray sources, 3 of which are previously unidentified. This cluster hosts a well-known bright low-mass X-ray binary, source A (or XB 1832-330). Source B shows…

高能天体物理现象 · 物理学 2015-05-28 G. Coomber , C. O. Heinke , H. N. Cohn , P. M. Lugger , J. E. Grindlay

We present near-infrared imaging and spectroscopic observations of two FR II high-redshift radio galaxies (HzRGs), 4C 40.36 (z=2.3) and 4C 39.37 (z=3.2), obtained with the Hubble, Keck, and Hale Telescopes. High resolution images were taken…

天体物理学 · 物理学 2009-11-07 E. Egami , L. Armus , G. Neugebauer , T. W. Murphy , B. T. Soifer , K. Matthews , A. S. Evans

We report the discovery of a $z\sim3.9$ protocluster identified from Atacama Large Millimetre/sub-millimetre Array Band 3 spectral scans of a bright radio source selected from the GaLactic and Extra-galactic All-sky Murchison Widefield…

星系天体物理 · 物理学 2025-06-13 A. J. Hedge , N. Seymour , J. W. Broderick , A. Gupta , J. Afonso , L. Ighina , M. Lehnert , G. Noirot , S. Shabala , D. Stern , R. J. Turner

This paper presents the first high-resolution and high-sensitivity study of the radio properties of optically selected type~2 quasars. We used the Very Large Array at 8.4 GHz to observe 59 sources drawn from the Sloan Digital Sky Survey…

宇宙学与河外天体物理 · 物理学 2015-05-14 Dharam Vir Lal , Luis C. Ho

Context. High redshift radio galaxies are among the most massive galaxies at their redshift, are often found at the center of protoclusters of galaxies, and are expected to evolve into the present day massive central cluster galaxies. Thus…

Luminous radio sources are thought to lie in galaxy clusters or proto-clusters. The complete sample of 64 high-redshift 3C sources at $1<z<2.5$ has been mapped with the Spitzer Space Telescope. The IRAC $3.6\mu$m and $4.5\mu$m 5-$\sigma$…

星系天体物理 · 物理学 2017-10-09 Z. Ghaffari , Ch. Westhues , M. Haas , R. Chini , S. P. Willner , M. L. N. Ashby , B. J. Wilkes

Recent deep Chandra observations of nearby Compton thick (CT) AGN have produced surprising results, uncovering extended emission not only in the soft X-rays but in the hard emission (>3 keV), challenging the long-held belief that the…

星系天体物理 · 物理学 2023-06-28 Anna Trindade Falcao , G. Fabbiano , M. Elvis , A. Paggi , W. P. Maksym

We report the discovery of extended X-ray emission around the powerful high-redshift quasar GB 1508+5714 at z=4.3, revealed in a long Chandra ACIS observation. The emission feature is 3-4 arcsec away from the quasar core, which corresponds…

天体物理学 · 物理学 2009-11-10 W. Yuan , A. C. Fabian , A. Celotti , P. G. Jonker

In this letter we report the detection of an extremely strong X-ray emission line in the 940ks chandra ACIS-I spectrum of CXO CDFS J033225.3-274219. The source was identified as a Type1 AGN at redshift of z = 1.617, with 2.0 -- 10.0 keV…

天体物理学 · 物理学 2015-06-24 J. Wang , T. Yaqoob , G. Szokoly , R. Gilli , L. Kewley , V. Mainieri , M. Nonino , P. Rosati , P. Tozzi , W. Zheng , A. Zirm , C. Norman

We present the radio and X-ray properties of 1.2 mm MAMBO source candidates in a 1600 sq. arcmin field centered on the Abell 2125 galaxy cluster at z=0.247. The brightest, non-synchrotron mm source candidate in the field has a photometric…

宇宙学与河外天体物理 · 物理学 2009-07-24 Jeff Wagg , Frazer Owen , Frank Bertoldi , Maike Sawitzki , Christopher L. Carilli , Karl M. Menten , Hauke Voss

We report the discovery of a galaxy overdensity at z=1.11 associated with the z=1.110 high-redshift radio galaxy MG0442+0202. The group, CL0442+0202, was found in a near-infrared survey of z>1 radio galaxies undertaken to identify…

天体物理学 · 物理学 2009-11-07 Daniel Stern , Brad Holden , S. A. Stanford , Hyron Spinrad

We present ASCA observations of LINERs without broad H$\alpha$ emission in their optical spectra. The sample of "type 2" LINERs consists of NGC 404, 4111, 4192, 4457, and 4569. We have detected X-ray emission from all the objects except for…

天体物理学 · 物理学 2009-10-31 Y. Terashima , L. C. Ho , A. F. Ptak , R. F. Mushotzky , P. J. Serlemitsos , T. Yaqoob , H. Kunieda

The 500ks Chandra ACIS-I observation of the field around the $z=6.31$ quasar SDSS J1030+0524 is currently the 5th deepest extragalactic X-ray survey. The rich multi-band coverage of the field allowed for an effective identification and…

We present new Chandra observations of 21 z>4 quasars, including 11 sources at z>5. These observations double the number of X-ray detected quasars at z>5, allowing investigation of the X-ray spectral properties of a substantial sample of…

We present Gemini integral field spectroscopy and Keck II longslit spectroscopy of the extended emission-line region (EELR) around the quasar 4C 37.43. The velocity structure of the ionized gas is complex and cannot be explained globally by…

天体物理学 · 物理学 2009-06-23 Hai Fu , Alan Stockton

We present X-ray observations of nine Weak-Line Radio Galaxies (WLRGs), optically classified as confirmed or possible Low Ionization Nuclear Emission-line Regions (LINERs). The data were taken from the Chandra, XMM, and BeppoSax archives.…

天体物理学 · 物理学 2009-11-10 Alexander S. Rinn , Rita M. Sambruna , Mario Gliozzi