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The basic state of the velocity field in the gas close to the galactic centre

Published online by Cambridge University Press:  14 August 2015

K. Rohlfs  and
Th. Schmidt-Kaler
K. Rohlfs
Affiliation:
Astronomisches Institut, Ruhr-Universität, Bochum, FRG
Th. Schmidt-Kaler
Affiliation:
Astronomisches Institut, Ruhr-Universität, Bochum, FRG

Extract

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To explain the features in the range 340° ≤ 1 ≤ 22° which show expansion velocities, elliptical stream-lines have been proposed that happen to expose expansion components towards the sun. Three general observations, however, make this interpretation doubtful:

Type
VI. THE GALACTIC NUCLEUS
Information
Symposium - International Astronomical Union , Volume 84: The Large-Scale Characteristics of the Galaxy , 1979 , pp. 393 - 394
Copyright
Copyright © Reidel 1979