Modelling optical emission of Ultra-luminous X-ray Sources accreting above the Eddington limit

Author:

Ambrosi Elena12,Zampieri Luca2

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

Cited by 18 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Comprehensive X-ray and multiwavelength study of ULXs in NGC 1566;Monthly Notices of the Royal Astronomical Society;2023-11-27

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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