Wright, D. J. ; De Cat, P. ; Pollard, K. R. ; Maisonneuve, F. ; Kilmartin, P. M. ; Telting, J. H. ; Kambe, E. ; Poretti, E. ; Lehmann, H. ; Yang, S. ; Mkrtichian, D. ; Laney, D. ; Fu, J. N.

published in American Institute of Physics Conference Series, 1170, pp. 467-473 (2009)

Abstract: As part of a observational project aiming to investigate the effects of rotation on main-sequence g-mode non-radial pulsation we have obtained at least one (generally more) high-resolution spectroscopic observation of more than 50 confirmed or candidate γ Doradus and slowly pulsating B stars and have completed a spectroscopic multi-site campaign. The campaign was one of those outlined in De Cat et al. (these proceedings) and included five observatories and focused on the γ Doradus, and now planet hosting star HD 218396 (HR 8799) and the SPB stars HD 21071 and HD 25558.

DOI: 10.1063/1.3246544
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