Amanote Research

Amanote Research

    RegisterSign In

Superluminal Motion in the Largest Known Quasar

Symposium - International Astronomical Union
doi 10.1017/s0074180900133790
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 1988

Authors
P. D. BarthelR. T. SchilizziG. K. MileyE. PreussJ. R. Hooimeyer
Publisher

Cambridge University Press (CUP)


Related search

Evolution of the Milliarcsecond Polarization Structure of the Superluminal Quasar 3C345

Symposium - International Astronomical Union
1988English

Superluminal Motion in CTA 102

Symposium - International Astronomical Union
1989English

Uniform Apparent Superluminal Motion in 4C39.25

Symposium - International Astronomical Union
1988English

4C39.25 – Superluminal Motion Between Stationary Components

Symposium - International Astronomical Union
1988English

A Hubble Constant Measurement From Superluminal Motion of the Jet in GW170817

Nature Astronomy
AstrophysicsAstronomy
2019English

Search for Superluminal Motion in the Weak Cores of Extended Quasars

Symposium - International Astronomical Union
1986English

Superluminal Motion in a Compact Steep Spectrum Radio Source 3C 138

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2001English

Shock Models of Time Variability and Superluminal Motion in Compact Extragalactic Radio Sources

Symposium - International Astronomical Union
1988English

Structure From Motion With Known Camera Positions

English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy