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Spectral luminosity indicators in SNe Ia — The R(Si II) line strength ratio

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Hachinger,  Stephan
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Mazzali,  Paolo A.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Hillebrandt,  Wolfgang
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Citation

Hachinger, S., Mazzali, P. A., Tanaka, M., Hillebrandt, W., & Benetti, S. (2009). Spectral luminosity indicators in SNe Ia — The R(Si II) line strength ratio. In G. Giobbi, A. Tornambe, G. Raimondo, M. Limongi, L. Antonelli, N. Menci, et al. (Eds.), Probing Stellar Populations out to the Distant Universe (pp. 573-576). Melville, NY, USA: American Institute of Physics.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-A44E-E
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