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Spatial closeness of the white hypergiants HD 168607 and HD 168625

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Abstract

Our spectroscopic monitoring of the hypergiants HD 168607 (B9.5 Ia-0) and HD 168625 (B5.5 Ia-0) with resolutions from 15000 to 70000 confirms that both stars belong to the Ser OB1 association, proves their spatial closeness, and increases the probability that they constitute a physical pair.

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Translated from Pis'ma v Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 30, No. 7, 2004, pp. 511–518.

Original Russian Text Copyright © 2004 by Chentsov, Gorda.

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Chentsov, E.L., Gorda, E.S. Spatial closeness of the white hypergiants HD 168607 and HD 168625. Astron. Lett. 30, 461–468 (2004). https://doi.org/10.1134/1.1774398

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