The AH Pictoris Syndrome: Continuous Trains of Stunted Outbursts in Novalike Variables
Novalike variables are a subgroup of cataclysmic variables (CVs) that—unlike dwarf novae—do not exhibit strong brightenings in their long-term light curves.
Albert Bruch
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Superoutbursts and Positive Superhumps Occurred during the Standstill of a Z Cam-type Dwarf Nova
Dwarf novae (DNe) are semidetached binaries, where a white dwarf accretes material from a cool main-sequence companion via an accretion disk, and are known for their intermittent outbursts, making them key systems for studying accretion physics.
Qi-Bin Sun +6 more
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Phosphorus-rich stars with unusual abundances are challenging theoretical predictions. [PDF]
Masseron T +6 more
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Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities. [PDF]
Rosati P +39 more
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Following the Pulsations in the Long-term Cooling of GW Librae and V386 Serpentis
GW Lib and V386 Ser are dwarf novae systems containing pulsating white dwarfs that underwent large 8–9 mag amplitude outbursts in 2007 and 2019, respectively.
Paula Szkody +5 more
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The fungus Kalmusia longispora is able to cause vascular necrosis on Vitis vinifera. [PDF]
Karácsony Z +4 more
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Cataclysmic and Close Binaries in Star Clusters. V. Erupting Dwarf Novae, Faint Blue Stars, X‐Ray Sources, and the Classical Nova in the Core of M80 [PDF]
Michael M. Shara +2 more
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Cluster Analysis of Presolar Silicon Carbide Grains: Evaluation of Their Classification and Astrophysical Implications. [PDF]
Boujibar A +11 more
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New Observational Frontiers of ER UMa (= PG 0943+521) Type Dwarf Novae [PDF]
Daisaku Nogami +6 more
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Common Envelopes, Gamma Rays, and Sudden Spectral Changes of Novae
A common envelope (CE) is proposed as the origin of the early post-outburst spectra of many novae. A simple model is proposed to explain the properties of the CE based on the emission line strengths and an assumed density distribution.
Robert Williams +2 more
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