Solving asymmetries in the HVC´s distribution

Title:

Solving asymmetries in the HVC´s distribution

Creator:

Bajaja, E., Morras, R., and Pöppel, W. G. L.

Identifier:

https://cdk.lib.cas.cz/client/handle/uuid:78d9c17f-44a2-4b76-881f-95ee612bd9b6
uuid:78d9c17f-44a2-4b76-881f-95ee612bd9b6

Subject:

radioastronomie, asymmetries, and high velocity clouds (HVC´s)

Type:

model:article and TEXT

Format:

bez média and svazek

Description:

A large sample of high velocity HI detections have been collected from several surveys of HCV´s. All detections of HI that could be associated with a known object were subtracted. The main asymmetries in the velocity-position diagrams, shown by the very high velocity component (VHVC´s) were apparently reproduced with a kinematical model which, in addition, could explain other pecullarities of the HCV´s distiribution. The parameters of this model indicate that the VHCV´s might be at distances of the order if the size of the Local Group of Galaxies.

Language:

Czech

Rights:

http://creativecommons.org/publicdomain/mark/1.0/
policy:public

Coverage:

237-239

Source:

Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1987 Volume:63-70 | Number:69

Harvested from:

CDK

Metadata only:

false