Open AccessA polarimetric study of the B[e] star HD 45677
Author(s) -
Patel M.,
Oudmaijer R. D.,
Vink J. S.,
Mottram J. C.,
Davies B.
Publication year - 2006
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2006.11124.x
Subject(s) - physics , polarization (electrochemistry) , polarimetry , astrophysics , emission spectrum , ionization , circular polarization , stars , astronomy , spectral line , optics , scattering , ion , chemistry , quantum mechanics , microstrip
We present new medium‐resolution spectropolarimetric observations of HD 45677 in the B and R bands. A change in polarization is detected across Hα, Hβ and Hγ confirming that the ionized region around the star is aspherical. ( Q , U ) points associated with these emission lines occur away from the continuum, defining a polarization vector which points in the same direction for each of the lines at an average intrinsic polarization angle of 164°± 3°. These data were combined with past photometric and polarimetric data from the literature to investigate any variability. We find that HD 45677 is both photometrically and polarimetrically variable and that these changes are linked. We suggest that these variations may be caused by an aspherical blowout, and by deriving a least‐squares fit to the B ‐band polarimetric data in the Q – U space, we show that the blowout occurs at an intrinsic polarization angle of 175°± 1°, along the same angle as the proposed geometry of the ionized region.