Observed properties of FRII quasars and radio galaxies at z < 1.0

L.M. Mullin; J.M. Riley; M.J. Hardcastle

doi:10.1111/j.1365-2966.2008.13534.x

Observed properties of FRII quasars and radio galaxies at z < 1.0

L.M. Mullin, J.M. Riley, M.J. Hardcastle

Research output: Contribution to journal › Article › peer-review

63 Citations (Scopus)

21 Downloads (Pure)

Original language	English
Pages (from-to)	595-621
Journal	Monthly Notices of the Royal Astronomical Society
Volume	390
Issue number	2
DOIs	https://doi.org/10.1111/j.1365-2966.2008.13534.x
Publication status	Published - 2008

Keywords

radio continuum
Faraday rotation
asymmetric depolarization

Access to Document

10.1111/j.1365-2966.2008.13534.x

902872.pdf

Cite this

@article{7c5bc6ba5f7042518d1f59d6de62f2ec,

title = "Observed properties of FRII quasars and radio galaxies at z < 1.0",

keywords = "radio continuum, Faraday rotation, asymmetric depolarization",

author = "L.M. Mullin and J.M. Riley and M.J. Hardcastle",

note = "The original article can be found at: http://www3.interscience.wiley.com Copyright Blackwell / RAS. DOI: 10.1111/j.1365-2966.2008.13534.x",

year = "2008",

doi = "10.1111/j.1365-2966.2008.13534.x",

language = "English",

volume = "390",

pages = "595--621",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press (OUP)",

number = "2",

}

TY - JOUR

T1 - Observed properties of FRII quasars and radio galaxies at z < 1.0

AU - Mullin, L.M.

AU - Riley, J.M.

AU - Hardcastle, M.J.

N1 - The original article can be found at: http://www3.interscience.wiley.com Copyright Blackwell / RAS. DOI: 10.1111/j.1365-2966.2008.13534.x

PY - 2008

Y1 - 2008

KW - radio continuum

KW - Faraday rotation

KW - asymmetric depolarization

U2 - 10.1111/j.1365-2966.2008.13534.x

DO - 10.1111/j.1365-2966.2008.13534.x

M3 - Article

SN - 0035-8711

VL - 390

SP - 595

EP - 621

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -