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12 papers · 2 filters
FAUST XXX: Dust enhancement in the young binary L1551 IRS 5
Nicolás Cuello, Eleonora Bianchi, François Ménard +17
Young binary stars with discs provide unique laboratories to study the earliest stages of planet formation in star-forming environments. The detection of substructure in discs arou…
Comparison of Ne-22 core and shell distilled WD detonations in AREPO
Uri Pierre Burmester, Lilia Ferrario, Ivo R. Seitenzahl +1
We present three-dimensional hydrodynamical simulations of detonations in white dwarfs that have undergone distillation during crystall…
Pre-supernova O-C shell mergers could produce more than the explosion
Joshua Issa, Falk Herwig
The formation of in massive stars is thought to occur during explosive nucleosynthesis, however recent studies have shown it can be produced during O-C shell mer…
Calcium Excess in Novae: Beyond Nuclear Physics Uncertainties
Mallory Loria, Pavel Denissenkov, Chris Ruiz +1
We examine Ca abundances in classical novae from spectroscopic observations spanning 65 years and investigate whether they are systematically high compared to those predicted by no…
FAUST. XXVIII. High-Resolution ALMA Observations of Class 0/I Disks: Structure, Optical Depths, and Temperatures
M. J. Maureira, J. E. Pineda, H. B. Liu +22
We present high-resolution (~7.5 au) ALMA observations at 1.3 and 3 mm of 16 disks around Class 0/I protostars across multiple star-forming regions and a variety of multiplicities,…
Production of radioactive Na in core-collapse supernovae: the Ne-E(L) component in presolar grains and its possible consequences on supernova observations
M. Pignatari, S. Amari, P. Hoppe +8
Presolar graphite grains carry the isotopic signatures of their parent stars. A significant fraction of presolar graphites shows isotopic abundance anomalies relative to solar for…