Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S272(6), p. 414-415, 2010
DOI: 10.1017/s1743921311010982
Full text: Unavailable
AbstractWe present preliminary results of a 4-month campaign carried out in the framework of the Mons project, where time-resolved Hα observations are used to study the wind and circumstellar properties of a number of OB stars.