Astronomy conference

The conference will focus on stellar objects at any evolutionary stage that currently manifest themselves as early-type stars with signs of gaseous and/or dusty circumstellar material through spectral line emission and infrared excess. This definition includes such classes of object as Herbig Ae/Be, classical Be, Vega-type, Wolf-Rayet stars, Proto-Planetary Nebulae, Luminous Blue Variables, other types of object with the B[e] phenomenon, and any other relevant objects with gaseous and dusty circumstellar material.   More details on the conference website