A&A 540, A91 (2012) Astronomy DOI: 10.1051/0004-6361/201117715 & c ESO 2012 Astrophysics The spectroscopic orbits and physical parameters of GG Carinae P. Marchiano 1,E.Brandi1,2,3, M. F. Muratore1, C. Quiroga1,2,O.E.Ferrer1,4, and L. G. García1,2 1 Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque S/N – 1900 La Plata, Buenos Aires, Argentina e-mail:
[email protected] 2 Instituto de Astrofísica de La Plata (CCT La Plata-CONICET-UNLP), Argentina 3 Comisión de Investigaciones Científicas de la Provincia de Buenos Aires, (CIC), Argentina 4 Consejo Nacional de Investigaciones Científicas y Técnicas, (CONICET), Argentina Received 15 July 2011 / Accepted 22 December 2011 ABSTRACT Aims. GG Car is an eclipsing binary classified as a B[e] supergiant star. The aims of our study are to improve the orbital elements of the binary system in order to obtain the actual orbital period of this system. We also compare the spectral energy distribution of the observed fluxes over a wide wavelength range with a model of a circumstellar envelope composed of gas and dust. This fitting allows us to derive the physical parameters of the system and its environment, as well as to obtain an estimation of the distance to GG Car. Methods. We analyzed about 55 optical and near infrared spectrograms taken during 1996–2010. The spectroscopic orbits were obtained by measuring the radial velocities of the blueshifted absorptions of the He I P-Cygni profiles, which are very representative of the orbital motion of both stars.