RXJ2314.9+2243 from radio to X-rays Virtual Observatory Resource

Authors
  1. Komossa S.
  2. Xu D.
  3. Fuhrmann L.
  4. Grupe D.
  5. Yao S.
  6. Fan Z.
  7. Myserlis I.,Angelakis E.
  8. Karamanavis V.
  9. Yuan W.
  10. Zensus J.A.
  11. Published by
    CDS
Abstract

Radio-loud narrow-line type 1 galaxies provide us with a fresh look at the blazar phenomenon, the causes of radio loudness, and the physics of jet formation. We present a multi-wavelength study of the radio-loud narrow-line type 1 quasar RX J2314.9+2243, which exhibits some remarkable multi-wavelength properties. It is among the few radio-loud narrow-line type 1 galaxies, with a tentative {gamma}-ray detection, is luminous in the infrared, and shows an exceptionally broad and blueshifted [OIII]{lambda}5007 emission-line component. In order to understand the nature of this source, we have obtained optical, UV, X-ray, and radio observations of RX J2314.9+2243.

Keywords
  1. quasars
  2. seyfert-galaxies
  3. spectroscopy
Bibliographic source Bibcode
2015A&A...574A.121K
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/574/A121
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/574/A121
Document Object Identifer DOI
doi:10.26093/cds/vizier.35740121

Access

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Web browser access HTML
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History

2015-02-04T06:40:07Z
Resource record created
2015-02-04T06:40:07Z
Created
2018-03-26T05:41:14Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr