Type Ia SNe along redshift: the R(Si II) ratio and the expansion velocities in 
intermediate-z supernovae

Altavilla, G.; Ruiz-Lapuente, P.; Balastegui, A.; Méndez, J.; Irwin, M.; Espana-Bonet, C.; Ellis, R. S.; Folatelli, G.; Goobar, A.; Hillebrandt, W.; McMahon, R. M.; Nobili, S.; Stanishev, V.; Walton, N. A.

doi:10.1088/0004-637X/695/1/135

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Type Ia SNe along redshift: the R(Si II) ratio and the expansion velocities in intermediate-z supernovae

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Ruiz-Lapuente, P.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Hillebrandt, W.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Altavilla, G., Ruiz-Lapuente, P., Balastegui, A., Méndez, J., Irwin, M., Espana-Bonet, C., Ellis, R. S., Folatelli, G., Goobar, A., Hillebrandt, W., McMahon, R. M., Nobili, S., Stanishev, V., & Walton, N. A. (2009). Type Ia SNe along redshift: the R(Si II) ratio and the expansion velocities in intermediate-z supernovae. The Astrophysical Journal, 695(1), 135-148. doi:10.1088/0004-637X/695/1/135.

引用: https://hdl.handle.net/11858/00-001M-0000-0011-A35D-7

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