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References
- 1 2 3 4 "AT 2018hyz | Transient Name Server". www.wis-tns.org.
- ↑ Cendes, Y.; Berger, E.; Alexander, K. D.; Gomez, S.; Hajela, A.; Chornock, R.; Laskar, T.; Margutti, R.; Metzger, B.; Bietenholz, M. F.; Brethauer, D.; Wieringa, M. H. (1 October 2022). "A Mildly Relativistic Outflow Launched Two Years after Disruption in Tidal Disruption Event AT2018hyz". The Astrophysical Journal. 938 (1): 28. arXiv: 2206.14297 . Bibcode:2022ApJ...938...28C. doi: 10.3847/1538-4357/ac88d0 .
- ↑ "'We've Never Seen Anything Like This Before:' Black Hole Spews Out Material Years After Shredding Star | Center for Astrophysics | Harvard & Smithsonian". www.cfa.harvard.edu. Retrieved 7 May 2024.
- ↑ Matsumoto, Tatsuya; Piran, Tsvi (2 May 2023). "Generalized equipartition method from an arbitrary viewing angle". Monthly Notices of the Royal Astronomical Society. 522 (3): 4565–4576. arXiv: 2211.10051 . doi: 10.1093/mnras/stad1269 .
- ↑ Gomez, Sebastian; Nicholl, Matt; Short, Philip; Margutti, Raffaella; Alexander, Kate D; Blanchard, Peter K; Berger, Edo; Eftekhari, Tarraneh; Schulze, Steve; Anderson, Joseph; Arcavi, Iair; Chornock, Ryan; Cowperthwaite, Philip S; Galbany, Lluís; Herzog, Laura J (2020-07-20). "The Tidal Disruption Event AT 2018hyz II: Light-curve modelling of a partially disrupted star". Monthly Notices of the Royal Astronomical Society. 497 (2): 1925–1934. doi: 10.1093/mnras/staa2099 . ISSN 0035-8711.
- 1 2 Short, P; Nicholl, M; Lawrence, A; Gomez, S; Arcavi, I; Wevers, T; Leloudas, G; Schulze, S; Anderson, J P; Berger, E; Blanchard, P K; Burke, J; Segura, N Castro; Charalampopoulos, P; Chornock, R (2020-09-02). "The tidal disruption event AT 2018hyz – I. Double-peaked emission lines and a flat Balmer decrement". Monthly Notices of the Royal Astronomical Society. 498 (3): 4119–4133. doi: 10.1093/mnras/staa2065 . ISSN 0035-8711.
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