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Cited article:

Multiwavelength Modeling the SED of Luminous Supersoft X-Ray Sources in Large Magellanic Cloud and Small Magellanic Cloud

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The Astronomical Journal 164 (4) 145 (2022)
https://doi.org/10.3847/1538-3881/ac897d

Linking the properties of accreting white dwarfs with the ionization state of their ambient medium

D Souropanis, A Chiotellis, P Boumis, et al.
Monthly Notices of the Royal Astronomical Society 513 (2) 2369 (2022)
https://doi.org/10.1093/mnras/stac890

Supersoft X-ray nebulae in the Large Magellanic Cloud

Diego A Farias, Alejandro Clocchiatti, Tyrone E Woods and Armin Rest
Monthly Notices of the Royal Astronomical Society 497 (3) 3234 (2020)
https://doi.org/10.1093/mnras/staa2213

Excluding supersoft X-ray sources as progenitors for four Type Ia supernovae in the Large Magellanic Cloud

J Kuuttila, M Gilfanov, I R Seitenzahl, T E Woods and F P A Vogt
Monthly Notices of the Royal Astronomical Society 484 (1) 1317 (2019)
https://doi.org/10.1093/mnras/stz065

The connection between the peaks in velocity dispersion and star-forming clumps of turbulent galaxies

P. Oliva-Altamirano, D. B. Fisher, K. Glazebrook, et al.
Monthly Notices of the Royal Astronomical Society 474 (1) 522 (2018)
https://doi.org/10.1093/mnras/stx2797

Where are all of the nebulae ionized by supersoft X-ray sources?

T. E. Woods and M. Gilfanov
Monthly Notices of the Royal Astronomical Society 455 (2) 1770 (2016)
https://doi.org/10.1093/mnras/stv2423

Progenitor constraints on the Type-Ia supernova SN2011fe from pre-explosion Hubble Space Telescope He ii narrow-band observations

Or Graur, Dan Maoz and Michael M. Shara
Monthly Notices of the Royal Astronomical Society: Letters 442 (1) L28 (2014)
https://doi.org/10.1093/mnrasl/slu052