The variable stellar wind of Rigel probed at high spatial and spectral resolution

@article{Chesneau2014TheVS,
  title={The variable stellar wind of Rigel probed at high spatial and spectral resolution},
  author={Olivier Chesneau and A. Kaufer and Otmar Stahl and C. Colvinter and Alain Spang and Luc Dessart and Raman K. Prinja and Rolf Chini},
  journal={Astronomy and Astrophysics},
  year={2014},
  volume={566}
}
Context. Luminous BA-type supergiants are the brightest stars in the visible that can be observed in distant galaxies and are potentially accurate distance indicators. The impact of the variability of the stellar winds on the distance determination remains poorly understood. Aims. Our aim is to probe the inhomogeneous structures in the stellar wind using spectro-interferometric monitoring. Methods. We present a spatially resolved, high-spectral resolution (R = 12 000) K-band temporal monitoring… 
Wind properties of variable B supergiants
Context. Variable B supergiants (BSGs) constitute a heterogeneous group of stars with complex photometric and spectroscopic behaviours. They exhibit mass-loss variations and experience different
Photospheric variability of the late B supergiant HD 199478
We present the results of spectral studies of the photospheric lines of the late B supergiant HD 199478 (B8 Iae) in the visual range. The radial velocities of photospheric lines, as well as the
Submilliarcsecond optical interferometry of the high-mass X-ray binary BP Cru with VLTI/GRAVITY
This is the final version. Available from American Astronomical Society via the DOI in this record

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