MERLIN observations of superluminal radio sources

I. W A Browne; R. R. Clark; P. K. Moore; T. W B Muxlow; P. N. Wilknson; M. H. Cohen; R. W. Porcas

doi:10.1038/299788a0

MERLIN observations of superluminal radio sources

I. W A Browne, R. R. Clark, P. K. Moore, T. W B Muxlow, P. N. Wilknson, M. H. Cohen, R. W. Porcas

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

Abstract

Powerful extragalactic radio sources may all be members of a single family in which those showing superluminal behaviour are the ones in which a relativistic jet is directed towards the observer. The superluminal sources are shown to have extended radio structures the form of which is consistent with such a unified scheme. This interpretation requires that the Hubble constant H0 should be nearer to 100 than to 50 km s-1 Mpc -1. © 1982 Nature Publishing Group.

Original language	English
Pages (from-to)	788-793
Number of pages	5
Journal	Nature
Volume	299
Issue number	5886
DOIs	https://doi.org/10.1038/299788a0
Publication status	Published - 1982

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title = "MERLIN observations of superluminal radio sources",

abstract = "Powerful extragalactic radio sources may all be members of a single family in which those showing superluminal behaviour are the ones in which a relativistic jet is directed towards the observer. The superluminal sources are shown to have extended radio structures the form of which is consistent with such a unified scheme. This interpretation requires that the Hubble constant H0 should be nearer to 100 than to 50 km s-1 Mpc -1. {\textcopyright} 1982 Nature Publishing Group.",

author = "Browne, {I. W A} and Clark, {R. R.} and Moore, {P. K.} and Muxlow, {T. W B} and Wilknson, {P. N.} and Cohen, {M. H.} and Porcas, {R. W.}",

year = "1982",

doi = "10.1038/299788a0",

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AU - Browne, I. W A

AU - Clark, R. R.

AU - Moore, P. K.

AU - Muxlow, T. W B

AU - Wilknson, P. N.

AU - Cohen, M. H.

AU - Porcas, R. W.

PY - 1982

Y1 - 1982

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AB - Powerful extragalactic radio sources may all be members of a single family in which those showing superluminal behaviour are the ones in which a relativistic jet is directed towards the observer. The superluminal sources are shown to have extended radio structures the form of which is consistent with such a unified scheme. This interpretation requires that the Hubble constant H0 should be nearer to 100 than to 50 km s-1 Mpc -1. © 1982 Nature Publishing Group.

U2 - 10.1038/299788a0

DO - 10.1038/299788a0

M3 - Article

SN - 0028-0836

VL - 299

SP - 788

EP - 793

JO - Nature

JF - Nature

IS - 5886

ER -

MERLIN observations of superluminal radio sources

Abstract

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