Are radio galaxies and quiescent galaxies different? Results from the analysis of HST brightness profiles

被引：0
|
作者：
机构：
[1] [1,De Ruiter, H.R.
[2] Parma, P.
[3] Capetti, A.
[4] 2,Fanti, R.
[5] Morganti, R.
[6] Santantonio, L.
来源：
De Ruiter, H.R. | 1600年 / EDP Sciences卷 / 439期
关键词：
60;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
引用
收藏
相关论文
共 50 条
  • [1] Are radio galaxies and quiescent galaxies different? Results from the analysis of HST brightness profiles
    de Ruiter, HR
    Parma, P
    Capetti, A
    Fanti, R
    Morganti, R
    Santantonio, L
    ASTRONOMY & ASTROPHYSICS, 2005, 439 (02) : 487 - U43
  • [2] SIZES AND SURFACE BRIGHTNESS PROFILES OF QUIESCENT GALAXIES AT z ∼ 2
    Szomoru, Daniel
    Franx, Marijn
    van Dokkum, Pieter G.
    ASTROPHYSICAL JOURNAL, 2012, 749 (02):
  • [3] RADIO SPECTRUM AND SURFACE BRIGHTNESS OF RADIO GALAXIES
    MALUMYAN, VG
    SOVIET ASTRONOMY LETTERS, 1990, 16 (04): : 290 - 291
  • [4] Quasar host galaxies: Recent results from HST
    Kukula, MJ
    MULTIWAVELENGTH AGN SURVEYS, 2004, : 373 - 378
  • [5] The Toomre sequence revisited with HST NICMOS:: Nuclear brightness profiles and colors of interacting and merging galaxies
    Rossa, Joern
    Laine, Seppo
    van der Marel, Roeland P.
    Mihos, J. Christopher
    Hibbard, John E.
    Boker, Torsten
    Zabludoff, Ann I.
    ASTRONOMICAL JOURNAL, 2007, 134 (06): : 2124 - 2147
  • [6] Stellar Mass Profiles of Quiescent Galaxies in Different Environments at z ∼ 0
    Mosleh, Moein
    Tavasoli, Saeed
    Tacchella, Sandro
    ASTROPHYSICAL JOURNAL, 2018, 861 (02):
  • [7] RADIO SPECTRA AND BRIGHTNESS DISTRIBUTIONS OF E GALAXIES AND SO-GALAXIES
    HEESCHEN, DS
    ASTROPHYSICAL LETTERS, 1970, 6 (01): : 49 - &
  • [8] HST and Keck observations of high redshift radio galaxies
    vanBreugel, WJM
    EXTRAGALACTIC RADIO SOURCES, 1996, (175): : 577 - 580
  • [9] HST observations of radio galaxies at Z similar to 1
    Best, PN
    COLD GAS AT HIGH REDSHIFT, 1996, 206 : 403 - 407
  • [10] RADIO BRIGHTNESS DISTRIBUTION OF 8 MARKARIAN GALAXIES
    SRAMEK, RA
    TOVMASSIAN, HM
    ASTROPHYSICAL JOURNAL, 1976, 207 (03): : 725 - &
12345