Modelling optical emission of Ultra-luminous X-ray Sources accreting above the Eddington limit
Author:
Affiliation:
1. Department of Physics and Astronomy, University of Padova, Italy
2. INAF-Astronomical Observatory of Padova, Italy
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/sty2213/25501111/sty2213.pdf
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2. The first glimpse of ULXs through the near-infrared images captured by the JWST;Monthly Notices of the Royal Astronomical Society;2023-11-02
3. Identification of Bubble Nebulae around NGC 55 ULX-1 with MUSE Observations;The Astrophysical Journal;2023-09-01
4. Identification of a Helium Donor Star in NGC 247 ULX-1;The Astrophysical Journal;2023-04-01
5. Possible optical counterparts of ULXs in NGC 1672;Astronomische Nachrichten;2023-02-07
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