Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2009-10-29
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
5 pages, 3 figures, accepted by Astronomy and Astrophysics
Scientific paper
Aims. We study the geometry of the circumstellar environment of the B[e] supergiant star GG Car. Methods. We present observations acquired using the IAGPOL imaging polarimeter in combination with the Eucalyptus-IFU spectrograph to obtain spectropolarimetric measurements of GG Car across Halpha at two epochs. Polarization effects along the emission line are analysed using the Q-U diagram. In particular, the polarization position angle (PA) obtained using the line effect is able to constrain the symmetry axis of the disk/envelope. Results. By analysing the fluxes, GG Car shows an increase in its double-peaked Halpha line emission relative to the continuum within the interval of our measurements (~43 days). The depolarization line effect around Halpha is evident in the Q-U diagram for both epochs, confirming that light from the system is intrinsically polarized. A rotation of the PA along Halpha is also observed, indicating a counter-clockwise rotating disk. The intrinsic PA calculated using the line effect (~85deg) is consistent between our two epochs, suggesting a clearly defined symmetry axis of the disk.
de Araújo Francisco Xavier
Domiciano de Souza Armando
Fernandes Marcelo Borges
Magalhaes Antonio Mario
Pereyra Antonio
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