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Cited article:

Enabling High Mass Accretion Rates Onto Massive Main Sequence Stars by Outer Envelope Mass Removal

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Considerations on the Origin of IRAS 19312+1950 Based on Long-term Maser Observations

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The Astrophysical Journal 981 (1) 41 (2025)
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On the Response of Massive Main Sequence Stars to Mass Accretion and Outflow at High Rates

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A Broad Line-width, Compact, Millimeter-bright Molecular Emission Line Source near the Galactic Center

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Nova 1670 (CK Vulpeculae) was a merger of a red giant with a helium white dwarf

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A bipolar structure and shocks surrounding the stellar-merger remnant V1309 Scorpii

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Rotation-tunnelling spectrum and astrochemical modelling of dimethylamine, CH3NHCH3, and searches for it in space

H S P Müller, R T Garrod, A Belloche, V M Rivilla, K M Menten, I Jiménez-Serra, J Martín-Pintado, F Lewen and S Schlemmer
Monthly Notices of the Royal Astronomical Society 523 (2) 2887 (2023)
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Envelope ejection and the transition to homologous expansion in common-envelope events

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A Rapidly Fading Star as a Type II Obscuring Intermediate Luminosity Optical Transient (ILOT) in a Triple-star System

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Spatiokinematic models of five nova remnants: correlations between nova shell axial ratio, expansion velocity, and speed class

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The mid-infrared environment of the stellar merger remnant V838 Monocerotis

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Explaining recently studied intermediate luminosity optical transients (ILOTs) with jet powering

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