Kinematics of relativistic ejection with Hubble flow.

Details Kinematics of relativistic ejection with Hubble flow. Kinematics of relativistic ejection with Hubble flow.

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.175...23g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 175, no. 1, Jan. 1991, p. 23-33.

Astronomy and Astrophysics

Astrophysics

1

Ejecta, Hubble Constant, Relativistic Velocity, Velocity Measurement, Cosmology, Red Shift

Scientific paper

What is observed as an apparent superluminal motion is the resultant velocity of Hubble flow and a local ejection. Taking Hubble flow into account can explain problems posed for the relativistic beaming model, such as the one-sidedness problem and the untolerable extension of the deprojected structure of some superluminal sources; the misalignment of small- and large-scale jets can be analyzed more appropriately. A significant by-product of the present investigation is a first step in finding a new way to determine the value of the Hubble constant, provided that the superluminal motion can be observed at much longer (meter) wavelengths.

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