论文标题
SN 2013F没有光度法的早期降压光度
Early bolometric luminosity of SN 2013fs without photometry
论文作者
论文摘要
提出了新的方法，用于基于一组H alpha发射在冲击突破后的第一天，基于一组H alpha发射光谱的超新星IIP重建。该方法利用了在宽Hα机翼中表现出的Preshock Interlar气体的辐射加速度的影响。在SN 2013F的情况下，该方法的效率是在冲击突破后6到10小时之间进行的。该方法的特殊特征是它不需要光度法，距离和灭绝。
The novel method is proposed for the reconstruction of the early bolometric light curve for supernovae IIP based on a set of spectra of H alpha emission during the first day after the shock breakout. The method exploits an effect of the radiative acceleration of the preshock circumstellar gas that is manifested in the broad H alpha wings. The efficiency of the method is demonstrated in the case of SN 2013fs with spectra taken between 6 and 10 hours after the shock breakout. The exceptional feature of this method is that it does not require the photometry, the distance, and the extinction.
