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Cited article:

CXO J004318.8+412016, a steady supersoft X-ray source in M 31

Marina Orio, G. J. M. Luna, R. Kotulla, et al.
Monthly Notices of the Royal Astronomical Society 470 (2) 2212 (2017)
https://doi.org/10.1093/mnras/stx1355

Diffuse gas in galaxies sheds new light on the origin of Type Ia supernovae

Jonas Johansson, Tyrone E. Woods, Marat Gilfanov, et al.
Monthly Notices of the Royal Astronomical Society 442 (2) 1079 (2014)
https://doi.org/10.1093/mnras/stu907

AN X-RAY AND OPTICAL LIGHT CURVE MODEL OF THE ECLIPSING SYMBIOTIC BINARY SMC3

Mariko Kato, Izumi Hachisu and Joanna Mikołajewska
The Astrophysical Journal 763 (1) 5 (2013)
https://doi.org/10.1088/0004-637X/763/1/5

A new super-soft X-ray source in the Small Magellanic Cloud: Discovery of the first Be/white dwarf system in the SMC?

R. Sturm, F. Haberl, W. Pietsch, et al.
Astronomy & Astrophysics 537 A76 (2012)
https://doi.org/10.1051/0004-6361/201117789

EVOLUTION OF THE SYMBIOTIC NOVA PU VUL—OUTBURSTING WHITE DWARF, NEBULAE, AND PULSATING RED GIANT COMPANION

Mariko Kato, Joanna Mikołajewska and Izumi Hachisu
The Astrophysical Journal 750 (1) 5 (2012)
https://doi.org/10.1088/0004-637X/750/1/5

Why are Supersoft X-ray Fluxes So Weak in Early-type Galaxies? – A Clue to Type Ia SNe Progenitors –

Mariko Kato
Proceedings of the International Astronomical Union 7 (S281) 145 (2011)
https://doi.org/10.1017/S1743921312014895