Properties and nature of Be stars - 28. Implications of systematic observations for the nature of the multiple system with the Be star o Cassiopeæ and its circumstellar environment

P. Koubský; C. A. Hummel; P. Harmanec; C. Tycner; F. van Leeuwen; S. Yang; M. Šlechta; H. Božić; R. T. Zavala; D. Ruždjak; D. Sudar

doi:10.1051/0004-6361/201014477

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Volume 517 (July 2010)

A&A, 517 (2010) A24

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Table B.3:

Observations in m₅₈ band of 13-C photometry.
HJD	m₅₈	Source
-2 400 000
39 745.8655	4.589	Mitchell & Johnson (1969)
44 500.9887	4.438	Schuster & Guichard (1984)
44 502.8917	4.465	$^{\prime\prime}$
44 503.8665	4.489	$^{\prime\prime}$
44 504.8761	4.511	$^{\prime\prime}$
44 980.9594	4.450	$^{\prime\prime}$
44 892.8040	4.504	$^{\prime\prime}$

Source LaTeX | All tables | In the text

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