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21 Pages

Discovering New B[e] Supergiants and Candidate Luminous Blue Variables in Nearby Galaxies

  • Grigoris Maravelias,
  • Stephan de Wit,
  • Alceste Z. Bonanos,
  • Frank Tramper,
  • Gonzalo Munoz-Sanchez and
  • Evangelia Christodoulou

Mass loss is one of the key parameters that determine stellar evolution. Despite the progress we have achieved over the last decades we still cannot match the observational derived values with theoretical predictions. Even worse, there are certain ph...

(This article belongs to the Special Issue Theory and Observation of Active B-type Stars)