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Table 7

Radii of the stars and roche lobe parameters.

i = 90°

Star ap (AU) aap (AU) m2 (M) R (R) RRLp (R) RRLap (R) RRGB/AGB (R) f

DY Ori 2.0 3.0 0.7 40 156 238 100 0.40.6
EP Lyr 0.9 3.8 0.7 36 74 297 112 0.41.5
HP Lyr 2.5 3.5 0.5 60 214 302 170 0.60.8
IRAS 17038 1.2 4.3 0.8 73 91 331 149 0.51.6
IRAS 09144 1.9 4.9 1.2 58 129 340 144 0.41.1
TW Cam 1.3 1.9 0.7 83 102 153 149 1.01.5

i = 60°

DY Ori 1.8 2.7 0.9 40 132 203 100 0.50.8
EP Lyr 0.8 3.4 0.9 36 63 253 112 0.41.8
HP Lyr 2.2 3.1 0.6 60 181 255 170 0.70.9
IRAS 17038 1.1 3.9 1.0 73 77 281 149 0.51.9
IRAS 09144 1.7 4.5 1.6 58 109 289 144 0.51.3
TW Cam 1.2 1.7 0.8 83 87 131 149 1.11.7

Notes. The orbital separation at periastron and apastron passage is shown in Cols. 2 and 3, respectively for two different inclinations of 90° and 60°. In Col. 4 we show the estimated masses of the companion assuming a primary mass of 0.6 M. Column 5 is the current radius of the primary derived from the effective temperature and luminosity. Columns 6 and 7 display the radius of the Roche lobe at periastron and apastron, respectively. Column 8 outlines the estimated radius of the star on the RGB/AGB, assuming an effective temperature of TRGB/AGB ~ 3500 K. We show the Roche lobe filling factors at apastron-periastron (f = RAGB/RRL or f = RRGB/RRL) in the last column.

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