Dr. Marcelo M. Miller Bertolami is a staff researcher at the Institute of Astrophysics in La Plata (IALP, UNLP-CONICET) and a teaching assistant in Special Relativity at the Faculty of Astronomy and Geophysics at the Universidad Nacional de La Plata (UNLP). He is also a member of the IAU Working Group on Red Giants and Supergiants and the editorial board of the AGB Newsletter. His main research interests are the final stages of the stellar evolution of low- and intermediate-mass stars. This includes the formation and evolution of central stars of planetary nebulae, white dwarfs, Hot-Subdwarf stars, stars in the asymptotic giant branch, and the study of stellar convection and pulsations in these stars.
Dr. Marcelo M. Miller Bertolami is a staff researcher at the Institute of Astrophysics in La Plata (IALP, UNLP-CONICET) and a teaching assistant in Special Relativity at the Faculty of Astronomy and Geophysics at the Universidad Nacional de La Plata (UNLP). He is also a member of the IAU Working Group on Red Giants and Supergiants and the editorial board of the AGB Newsletter. His main research interests are the final stages of the stellar evolution of low- and intermediate-mass stars. This includes the formation and evolution of central stars of planetary nebulae, white dwarfs, Hot-Subdwarf stars, stars in the asymptotic giant branch, and the study of stellar convection and pulsations in these stars.