中文
相关论文

相关论文: A jet-cloud interaction in 3C34 at redshift z = 0.…

200 篇论文

To properly understand the evolution of high-redshift galaxy clusters, both passive and star-forming galaxies have to be considered. Here we study the clustering environment of 21 radio galaxies and quasars at 1<z<2.5 from the third…

We report the results from a six-year, multi-epoch very long baseline interferomertry monitoring of the Seyfert galaxy NGC3079. We have observed NGC3079 during eight epochs between 1999 and 2005 predominantly at 5GHz, but covering the…

天体物理学 · 物理学 2008-11-26 Enno Middelberg , Ivan Agudo , Alan L. Roy , Thomas P. Krichbaum

A2319 is a massive, merging galaxy cluster with a previously detected radio halo that roughly follows the X-ray emitting gas. We present the results from recent observations of A2319 at 20 cm with the Jansky Very Large Array (VLA) and a…

高能天体物理现象 · 物理学 2015-06-23 Emma Storm , Tesla E. Jeltema , Lawrence Rudnick

Imaging at 1.25 and 2.20 microns has been obtained of the field containing the galaxy (RD1) found at redshift 5.34 by Dey et al.(1998). This galaxy has been detected at 1.25 microns, while the lower redshift (z=4.02) galaxy also found in…

天体物理学 · 物理学 2009-10-30 L. Armus , K. Matthews , G. Neugebauer , B. T. Soifer

We present the results of K-band imaging polarimetry of seven 3CR radio galaxies at redshifts (z) between 0.7 and 1.2. We find strong evidence for polarization in three sources: 3C 22, 3C 41 and 3C 114. Of these, 3C 41 shows strong evidence…

天体物理学 · 物理学 2009-10-30 G. Leyshon , Stephen A. Eales

Cross-correlating the Planck High Frequency Instrument (HFI) maps against quasars from the Sloan Digital Sky Survey (SDSS) DR7, we estimate the intensity distribution of the Cosmic Infrared Background (CIB) over the redshift range 0 < z <…

宇宙学与河外天体物理 · 物理学 2014-12-05 Samuel J. Schmidt , Brice Ménard , Ryan Scranton , Christopher B. Morrison , Mubdi Rahman , Andrew M. Hopkins

We combine new data from the Karl G. Jansky Very Large Array with previous radio observations to create a more complete picture of the ongoing interactions between the radio jet from galaxy NGC 541 and the star-forming system known as…

高能天体物理现象 · 物理学 2022-09-14 C. Nolting , M. Lacy , S. Croft , P. C. Fragile , S. T. Linden , K. Nyland , P. Patil

We present Hubble Space Telescope images of 11 high redshift radio galaxies (between $z=2.3$ and $z=3.6$). The galaxies were observed with the WFPC2 camera in a broad band filter (F606W or F707W, roughly equivalent to V or R-band), for 2…

We report a discovery of a large-scale bent radio jet in the merging galaxy cluster Abell 514 ($z = 0.071$). The radio emission originates from the two radio lobes of the AGN located near the center of the southern subcluster and extends…

星系天体物理 · 物理学 2023-10-03 Wonki Lee , John ZuHone , M. James Jee , Kim HyeongHan , Ruta Kale , Eunmo Ahn

We present results of Hubble Space Telescope observations of the radio galaxy 3C 244.1. The broadband F702W (R) and F555W (V) images (WFPC2/PC) show an elliptical galaxy and gaseous filaments and blobs surrounding it. In the narrow-band…

天体物理学 · 物理学 2009-11-07 Carlos Feinstein , F. Duccio Macchetto , Andre R. Martel , William B. Sparks

We present new observations with the Karl G. Jansky Very Large Array of seven X-ray-selected tidal disruption events (TDEs). The radio observations were carried out between 9 and 22 years after the initial X-ray discovery, and, thus, probe…

高能天体物理现象 · 物理学 2015-06-11 Geoffrey C. Bower , Brian D. Metzger , S. Bradley Cenko , Jeffrey M. Silverman , Joshua S. Bloom

Updates are provided on several issues related to Unified Models. A new HST spectrum of Cygnus A confirms the broad MgII emission line, and suggests a very large velocity width as seen in the polarized optical lines. Statistics of the 3CR…

天体物理学 · 物理学 2007-05-23 Robert Antonucci

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…

We analyze the optical spectra of massive (log M*/Msun > 11.4) radio-loud galaxies at z~0.2 and z~0.6. By comparing stellar population parameters of these radio-loud samples with radio-quiet control samples, we investigate how the presence…

The results of a deep spectroscopic campaign on powerful radio galaxies with redshifts z ~ 1, to investigate in detail their emission line gas properties, are presented. Both the 2-dimensional velocity structure of the [OII] 3727 emission…

天体物理学 · 物理学 2007-05-23 P. N. Best , H. J. A. R"ottgering , M. S. Longair

We present a detailed analysis of the gas conditions in the H_2 luminous radio galaxy 3C326N at z~0.1, which has a low star formation rate (SFR~0.07 M_sun/yr) in spite of a gas surface density similar to those in starburst galaxies. Its…

宇宙学与河外天体物理 · 物理学 2015-05-18 N. P. H. Nesvadba , F. Boulanger , P. Salome , P. Guillard , M. D. Lehnert , P. Ogle , P. Appleton , E. Falgarone , G. Pineau des Forets

II Zw 40 is a starburst dwarf and merger product, and holds a radio-infrared supernebula excited by thousands of embedded OB stars. We present here observations of three aspects of the supernebula: maps of the K and KU radio continuum that…

星系天体物理 · 物理学 2024-10-24 Dan Beilis , Sara Beck , John Lacy , Jean L. Turner , Hauyu Baobab Liu , Paul T. P. Ho , S. Michelle Consiglio

We present new {\it Chandra} observations of the radio galaxy 3C 445, centered on its southern radio hotspot. Our observations detect X-ray emission displaced upstream and to the west of the radio-optical hotspot. Attempting to reproduce…

高能天体物理现象 · 物理学 2014-11-20 Eric S. Perlman , Markos Georganopoulos , Emily M. May , Demosthenes Kazanas

In March 2018, Mukherjee (2018) reported the detection by VERITAS of very-high-energy emission (VHE; > 100 GeV) from 3C 264. This is the sixth, and second most distant, radio galaxy ever detected in the TeV regime. In this article we…

高能天体物理现象 · 物理学 2019-07-10 B. Boccardi , G. Migliori , P. Grandi , E. Torresi , F. Mertens , V. Karamanavis , R. Angioni , C. Vignali

We report here on the discovery of a red quasar, J004929.4+351025.7 at a redshift of z = 2.48, situated within a large Lya emission-line halo. The radio spectral energy distribution implies that the radio jets were triggered < 10^4 years…