Corona evolution of MAXI J1535‑571 revealed by type-C quasi-periodic oscillations observed with Insight-HXMT. Zhang, Y., Mendez, M., Garcı́a, Federico, Zhang, S., Karpouzas, K., Altamirano, D., Belloni, T., Qu, J., Zhang, S., Tao, L., Zhang, L., Huang, Y., Kong, L., Ma, R., Yu, W., Rawat, D., & Bellavita, C. In 44th COSPAR Scientific Assembly. Held 16-24 July, volume 44, pages 2359, July, 2022. bibtex @INPROCEEDINGS{2022cosp...44.2359Z,
author = {{Zhang}, Yuexin and {Mendez}, Mariano and {Garc{\'\i}a}, Federico and {Zhang}, Shuang-Nan and {Karpouzas}, Konstantinos and {Altamirano}, Diego and {Belloni}, Tomaso and {Qu}, Jinlu and {Zhang}, Shu and {Tao}, Lian and {Zhang}, Liang and {Huang}, Yue and {Kong}, Lingda and {Ma}, Ruican and {Yu}, Wei and {Rawat}, Divya and {Bellavita}, Candela},
title = "{Corona evolution of MAXI J1535‑571 revealed by type-C quasi-periodic oscillations observed with Insight-HXMT}",
booktitle = {44th COSPAR Scientific Assembly. Held 16-24 July},
year = 2022,
volume = {44},
month = jul,
pages = {2359},
adsurl = {https://ui.adsabs.harvard.edu/abs/2022cosp...44.2359Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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