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14. Comments on McClain's observations of IAU 17S2A
Published online by Cambridge University Press: 14 August 2015
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Reference to Fig. 1, p. 20 of this symposium will show that a 1° beam directed toward the galactic centre receives a range of velocities that is not negligible. This is due to galactic rotation, which causes material in one edge of the beam to approach and in the other edge to recede.
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- Part I: Spectral Line Investigations
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- Copyright © Cambridge University Press 1957
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