Millinovae: A New Class of Transient Supersoft X-Ray Sources Without a Classical Nova Eruption
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Przemek Mróz et al 2024 ApJL 977 L37 The discovery of 29 stars with properties similar to the enigmatic ASASSN-16oh suggests the existence of a class of white dwarfs with optical emission 1,000 fainter than classical novae. The post Millinovae: A New Class of Transient Supersoft X-Ray Sources Without a Classical Nova Eruption appeared first on AAS Nova .
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