Post-AGB stars with hot circumstellar dust: binarity of the low-amplitude pulsators

H. Van Winckel; T. Lloyd Evans; M. Briquet; P. De Cat; P. Degroote; W. De Meester; J. De Ridder; P. Deroo; M. Desmet; R. Drummond; L. Eyer; M. A. T. Groenewegen; K. Kolenberg; D. Kilkenny; D. Ladjal; K. Lefever; T. Maas; F. Marang; P. Martinez; R. H. Østensen; G. Raskin; M. Reyniers; P. Royer; S. Saesen; K. Uytterhoeven; J. Vanautgaerden; B. Vandenbussche; F. van Wyk; M. Vučković; C. Waelkens; W. Zima

doi:10.1051/0004-6361/200912332

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Volume 505 / No 3 (October III 2009)

A&A, 505 3 (2009) 1221-1232

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Table 8:

The evaluation of the mass of the invisible companion of every programme star.
Star	Mass of the companion in solar mass.
	i = 90 $^{\circ}$	i = 65 $^{\circ}$
IRAS 08544-4431	0.29	0.33
IRAS 12222-4652	0.13	0.15
EN TrA	1.25	1.50
IRAS 15469-5311	0.41	0.47
IRAS 19125+0343	0.49	0.56
IRAS 19157-0247	0.13	0.15

Source LaTeX | All tables | In the text

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