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ABSTRACT We study the properties of low–velocitymaterial in the line of sight towards nearby Type Ia Supernovae (SNe Ia) that have measured late phase nebular velocity shifts (vneb), thought to be an environment–independent observable. We have found that the distribution of equivalent widths of n...


Forster, FranciscoGonzález–Gaitán, SantiagoAnderson, JosephMarchi, SebastiánGutiérrez, Claudia P.Hamuy, MarioPignata, GiulianoCartier, Régis[Evidence for asymmetric distribution of circumstellar material around type ia supernovae.]Evidence for asymmetric distribution of circumstellar material around type ia supernovae.

We have detected, for the first time, Cepheid variables in the Sculptor Group spiral galaxy NGC 7793. From wide-field images obtained in the optical V and I bands on 56 nights in 2003-2005, we have discovered 17 long-period (24-62 days) Cepheids whose periods and mean magnitudes define tight per...


Pietrzynski, GrzegorzGieren, WolfgangHamuy, MarioPignata, GiulianoSoszynski, IgorUdalski, AndrzejWalker, AlistairFouque, PascalBresolin, FabioKudritzki, Rolf-Peter[The Araucaria Project. First Cepheid Distance to the Sculptor Group Galaxy NGC 7793 from Variables discovered in a Wide-Field Imaging Survey]The Araucaria Project. First Cepheid Distance to the Sculptor Group Galaxy NGC 7793 from Variables discovered in a Wide-Field Imaging Survey

From a sample of 12 well-observed Type Ia supernovae, we find clear evidence of correlations between early phase (U − B), (V − R), and (V − I) colors and the velocity shifts of the [Fe II] λ7155 and [Ni II] λ7378 nebular lines measured from late-phase spectra. As these lines are thought to trace t...


Cartier, RegisFoster, FranciscoCoppi, PaoloHamuy, MarioMaeda, KeiichiPignata, GuilianoFolatelli, Gastón[A study of the color diversity around maximum light in Type Ia supernovae]A study of the color diversity around maximum light in Type Ia supernovae

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