A Search for Possible Stellar Members of the α-Spiral Arm

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The proper motions of groups of stars, selected according to magnitude and colour, near (l, b.)=(140°, 0°), were analysed in an attempt to identify possible members of the α-spiral arm defined by Verschuur from Hi observations. Other than late type giants the only objects whose distance corresponded to that of this arm were a small group of reddened early type stars.

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