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KINEMATICS OF RELATIVISTIC EJECTION WITH HUBBLE FLOW .1. APPLICATORS TO SUPERLUMINAL MOTION
GONG, SM
1991
Source PublicationASTROPHYSICS AND SPACE SCIENCE
ISSN0004-640X
Volume175Issue:1Pages:23-33
AbstractWhat we observe as an apparent superluminal motion is the resultant velocity of Hubble flow and a local ejection. Taking Hubble flow into account, on 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 the initiation to find a new way to determine the value of the Hubble constant H0, provided that one can observe the superluminal motion at much longer wavelengths, say, meter wavelengths.
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8566
Collection期刊(老文献)
Recommended Citation
GB/T 7714
GONG, SM. KINEMATICS OF RELATIVISTIC EJECTION WITH HUBBLE FLOW .1. APPLICATORS TO SUPERLUMINAL MOTION[J]. ASTROPHYSICS AND SPACE SCIENCE,1991,175(1):23-33.
APA GONG, SM.(1991).KINEMATICS OF RELATIVISTIC EJECTION WITH HUBBLE FLOW .1. APPLICATORS TO SUPERLUMINAL MOTION.ASTROPHYSICS AND SPACE SCIENCE,175(1),23-33.
MLA GONG, SM."KINEMATICS OF RELATIVISTIC EJECTION WITH HUBBLE FLOW .1. APPLICATORS TO SUPERLUMINAL MOTION".ASTROPHYSICS AND SPACE SCIENCE 175.1(1991):23-33.
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