1996PASP..108..967V


Query : 1996PASP..108..967V

1996PASP..108..967V - Publ. Astron. Soc. Pac., 108, 967-971 (1996/November-0)

Is the eclipsing binary EU Hydrae a semi-detached system?

VIVEKANANDA RAO P., SARMA M.B.K. and ABHYANKAR K.D.

Abstract (from CDS):

The V and B light curves of the Algol type eclipsing binary EU Hydrae (EU Hya) obtained during 1973-74 and 1977 with the 1.2m telescope of the Japal-Rangapur Observatory were analyzed for elements using Wilson-Devinney synthetic light curve method. The results suggest that EU Hya is a semi detached system with a photometric mass ratio of 0.212. The primary component is found to be an F2V (6900 K) and the secondary component is an evolved star of K0-4V-IV (4152 K) spectral types.

Abstract Copyright: ∼

Journal keyword(s): Stars

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* HU Tau SB* 04 38 15.8301628464 +20 41 05.009485236   5.830 5.842     B8V 151 0
2 V* R CMa SB* 07 19 28.1785241208 -16 23 42.895279824 6.09 6.05 5.70     F2III/IV 290 0
3 V* EU Hya EB* 08 42 03.5665604160 -06 43 49.403320320   10.71 10.26     F6(N) 37 0
4 V* TT Hya SB* 11 13 12.4976326464 -26 27 54.253972800   7.43 7.31     F0IV:kA2mA3:_sh 193 0

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