2606.10011
2026-07-16
astro-ph.HE
版本更新
50%
A Multi-Wavelength View of the First Type Ic-BL Supernova with an Einstein Probe X-ray Shock Breakout
首次具有爱因斯坦探针X射线激波暴发的Ic-BL型超新星的多波段视角
Jillian C. Rastinejad, Gokul Srinivasaragavan, Nikhil Sarin, Tanner O'Dwyer, S. Bradley Cenko, James K. Leung, Anya E. Nugent, Daniel A. Perley, Genevieve Schroeder, Shreya Anand, Tomas Ahumada, Igor Andreoni, Aleksandra Bochenek, Alessandra Corsi, Christoffer Fremling, Anna Y. Q. Ho, Mansi M. Kasliwal, Geoffrey Mo, Anirudh Salgundi, Kendall I. Sippy, J. Sollerman, Eric C. Bellm, Tracy X. Chen, Michael W. Coughlin, Michael C. Davis, Fabio De Colle, Danielle Frostig, Christopher L. Fryer, Michael J. Graham, Xander J. Hall, K. -R. Hinds, Luca Izzo, Wynn Jacobson-Galan, Nathan P. Lourie, Keiichi Maeda, Josiah Purdum, Ben Rusholme, Avinash Singh, Robert Stein
专题命中
扩散模型
:diffusion(abstract)
AI总结
基于爱因斯坦探针发现的近邻快速X射线暂现源EP260321a,通过多波段观测确认其与Ic-BL型超新星SN 2026gzf成协,首次为这类超新星提供确凿的X射线激波暴发证据,并约束了喷流能量和射电辐射。