Secondary Maximum in the Near‐Infrared Light Curves of Type Ia Supernovae

ASTROPHYSICAL JOURNAL, no. 2 (2006): 939-953

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We undertake a theoretical study of the near-infrared (NIR) light curves of Type Ia supernovae (SNe Ia). In these bands, the light curves are distinguished by a secondary maximum occurring roughly 20-30 days after the initial one. Using time-dependent multigroup radiative transfer calculations, we calculate the UBVRIJHK-band light curves ...更多

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