Key points are not available for this paper at this time.
Abstract We present ultraviolet/optical/near-infrared observations and modeling of Type II supernovae (SNe II) whose early time ( δ t t IIn ≈ 3.8 M ̇ / (0.01 M ⊙ yr −1 ) days.
Jacobson-Galán et al. (Wed,) studied this question.