IAU 281 Poster MSWord no INAF - INAF

IAU Symposium 281
Binary Paths to Type Ia Supernovae Explosions
Padova, Italy • July 4 – 8 2011
Clues to progenitors from the environments of SNe Ia
and from delay times • SNe Ia and novae rates in
different galaxy types • Close binary secular evolution
and mass transfer • Thermonuclear flashes and nova
winds • Recurrent novae and symbiotics on the SNe Ia
path • Supersoft X-ray sources and hydrogen-burning white
dwarfs • Massive binaries as a new class of SNe Ia progenitors
• Tracking the progenitors using large surveys G. Galletta
 S O C  G. C. Anupama (India) & Marina Orio (Italy, USA) co-chairs, Şölen Balman
(Turkey), Lars Bildsten (USA), Rosanne Di Stefano (USA), Jeno Sokoloski (USA),
Paula Szkody (USA), Domitilla de Martino (Italy), Laura Greggio (Italy), Lilia Ferrario
(Australia), Rosario Gonzalez Riestra (Spain), Margarita Hernanz (Spain),
Pilar Ruiz Lapuente (Spain), Mariko Kato (Japan), Rubina Kotak (UK),
Joanna Mikolajewska (Poland), Dina Prialnik (Israel)
 L O C  Marina Orio (INAF Padova & U Wisconsin) & Rosanna Maregini Strunce
(Madison) co-chairs, Antonio Bianchini (U Padova & Planetario di Padova), Stefano Ciroi
(U Padova), Valentina Cracco (U Padova), Renato Falomo (INAF Padova & Planetario di
Padova), Daniela Faro (INAF Padova), Carmen Fasolato (Padova), Anita Makuluni
(U Wisconsin & Astronomical Journal), Elvira De Poli (Planetario di Padova),
Valeria Zanini (INAF Padova) Web: http://www.oapd.inaf.it/oapd/IAU281/IAU281.html
Email: [email protected]