Extended and compact X-ray emission in powerful radio galaxies

D. M. Worrall; C. R. Lawrence; T. J. Pearson; A. C. S. Readhead

Extended and compact X-ray emission in powerful radio galaxies

D. M. Worrall
, C. R. Lawrence
, T. J. Pearson
, A. C. S. Readhead

School of Physics

Research output: Contribution to journal › Article (Academic Journal) › peer-review

Abstract

We report ROSAT X-ray observations of two powerful radio galaxies. 3C 280 provides evidence for a mixture of unresolved and extended emission, with the latter produced by hot plasma of insufficient pressure to confine the radio lobes and insufficient density for a cooling flow to have begun. 3C 220.3 gives only an X-ray upper limit, but one consistent with our interpretation of the X-ray emission from powerful radio-loud active galactic nuclei (AGNs) in terms of obscured and unobscured components.

Original language	English
Journal	Astrophysical Journal Letters
Volume	420
Publication status	Published - 1 Jan 1994

Keywords

Active Galaxies
High Temperature Plasmas
Quasars
Radio Galaxies
X Ray Astronomy
X Rays
Computer Programs
Heao 2
Proportional Counters
Red Shift
Rosat Mission

Access to Document

http://adsabs.harvard.edu/abs/1994ApJ...420L..17W

Handle.net

Persistent link

Cite this

@article{9e12937f2df6451f87434b4c2f299d1b,

title = "Extended and compact X-ray emission in powerful radio galaxies",

abstract = "We report ROSAT X-ray observations of two powerful radio galaxies. 3C 280 provides evidence for a mixture of unresolved and extended emission, with the latter produced by hot plasma of insufficient pressure to confine the radio lobes and insufficient density for a cooling flow to have begun. 3C 220.3 gives only an X-ray upper limit, but one consistent with our interpretation of the X-ray emission from powerful radio-loud active galactic nuclei (AGNs) in terms of obscured and unobscured components.",

keywords = "Active Galaxies, High Temperature Plasmas, Quasars, Radio Galaxies, X Ray Astronomy, X Rays, Computer Programs, Heao 2, Proportional Counters, Red Shift, Rosat Mission",

author = "Worrall, \{D. M.\} and Lawrence, \{C. R.\} and Pearson, \{T. J.\} and Readhead, \{A. C. S.\}",

year = "1994",

month = jan,

day = "1",

language = "English",

volume = "420",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "American Astronomical Society",

}

TY - JOUR

T1 - Extended and compact X-ray emission in powerful radio galaxies

AU - Worrall, D. M.

AU - Lawrence, C. R.

AU - Pearson, T. J.

AU - Readhead, A. C. S.

PY - 1994/1/1

Y1 - 1994/1/1

N2 - We report ROSAT X-ray observations of two powerful radio galaxies. 3C 280 provides evidence for a mixture of unresolved and extended emission, with the latter produced by hot plasma of insufficient pressure to confine the radio lobes and insufficient density for a cooling flow to have begun. 3C 220.3 gives only an X-ray upper limit, but one consistent with our interpretation of the X-ray emission from powerful radio-loud active galactic nuclei (AGNs) in terms of obscured and unobscured components.

AB - We report ROSAT X-ray observations of two powerful radio galaxies. 3C 280 provides evidence for a mixture of unresolved and extended emission, with the latter produced by hot plasma of insufficient pressure to confine the radio lobes and insufficient density for a cooling flow to have begun. 3C 220.3 gives only an X-ray upper limit, but one consistent with our interpretation of the X-ray emission from powerful radio-loud active galactic nuclei (AGNs) in terms of obscured and unobscured components.

KW - Active Galaxies

KW - High Temperature Plasmas

KW - Quasars

KW - Radio Galaxies

KW - X Ray Astronomy

KW - X Rays

KW - Computer Programs

KW - Heao 2

KW - Proportional Counters

KW - Red Shift

KW - Rosat Mission

M3 - Article (Academic Journal)

SN - 2041-8205

VL - 420

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

ER -

Extended and compact X-ray emission in powerful radio galaxies

Abstract

Keywords

Access to Document

Handle.net

Fingerprint

Cite this