Neil Gehrels Swift天文台对超软新星的研究
高能天体物理现象
2020-08-05 v1
摘要
Neil Gehrels Swift天文台的快速响应能力，加上其观测计划的每日安排，使其成为在X射线和紫外波段跟踪新星的理想任务，尤其是在其快速演化的早期阶段以及整个超软源区间。许多经典和再发新星已在超软阶段及后续衰落过程中被Swift广泛监测。我们在此收集了2006年初至2017年底期间爆发的新星的观测结果。
引用
@article{arxiv.1908.02004,
title = {Neil Gehrels Swift Observatory studies of supersoft novae},
author = {K. L. Page and A. P. Beardmore and J. P. Osborne},
journal= {arXiv preprint arXiv:1908.02004},
year = {2020}
}
备注
54 pages, 33 figure panels, 2 tables. To be published in a Special Issue of Advances in Space Research, entitled "Nova Eruptions, Cataclysmic Variables and Related Systems: observational vs theoretical challenges in the 2020 era", following COSPAR 2018