借助INTEGRAL理解大质量X射线双星的研究进展与未来方向
高能天体物理现象
2021-02-17 v1
摘要
大质量X射线双星是银河系及邻近星系中最亮的X射线源之一。由于其高度变化的辐射与复杂的现象学，自X射线天文学诞生以来便吸引了高能天体物理界的兴趣。近年间，它们挑战了我们对从红外到甚高能众多能段中物理过程的理解。在本综述中，我们广泛而简洁地总结了主导大质量X射线双星在几乎全电磁波段辐射的物理过程。这些包括恒星风与致密天体强引力场和磁场的相互作用、极端磁与引力条件下物质的行为，以及大质量恒星因处于双星系统而受到的演化过程扰动。我们强调INTEGRAL任务在发现大质量X射线双星类中许多最有趣天体方面的作用，及其在过去二十年间重燃对这些源兴趣的贡献。我们展示INTEGRAL的发现不仅显著增加了已知大质量X射线双星的数量、从而推进了对整体群体的理解，还开启了新的研究窗口，促进了如今多数天体物理研究领域常见的多波段方法。我们以概述从X射线到甚高能域规划中的未来设施作结，它们有望帮助我们回答INTEGRAL科学观测逾18年后仍悬而未决的诸多问题。
引用
@article{arxiv.2009.03244,
title = {Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions},
author = {Peter Kretschmar and Felix Fürst and Lara Sidoli and Enrico Bozzo and Julia Alfonso-Garzón and Arash Bodaghee and Sylvain Chaty and Masha Chernyakova and Carlo Ferrigno and Antonios Manousakis and Ignacio Negueruela and Konstantin Postnov and Adamantia Paizis and Pablo Reig and José Joaquín Rodes-Roca and Sergey Tsygankov and Antony J. Bird and Matthias Bissinger né Kühnel and Pere Blay and Isabel Caballero and Malcolm J. Coe and Albert Domingo and Victor Doroshenko and Lorenzo Ducci and Maurizio Falanga and Sergei A. Grebenev and Victoria Grinberg and Paul Hemphill and Ingo Kreykenbohm and Sonja Kreykenbohm né Fritz and Jian Li and Alexander A. Lutovinov and Silvia Martínez-Núñez and J. Miguel Mas-Hesse and Nicola Masetti and Vanessa A. McBride and Andrii Neronov and Katja Pottschmidt and Jérôme Rodriguez and Patrizia Romano and Richard E. Rothschild and Andrea Santangelo and Vito Sguera and Rüdiger Staubert and John A. Tomsick and José Miguel Torrejón and Diego F. Torres and Roland Walter and Jörn Wilms and Colleen A. Wilson-Hodge and Shu Zhang},
journal= {arXiv preprint arXiv:2009.03244},
year = {2021}
}
备注
61 pages, 22 figures, 1 table, will be published in New Astronomy Reviews