Moin,
https://arxiv.org/abs/1805.06892
Empirically determined dilution factors of stripped-envelope, core-collapse SNe: Paper II – Using GRB-SNe to determine the Hubble Constant
https://arxiv.org/abs/1805.06897
SNe Kicks in Hierarchical Triple Systems
https://arxiv.org/abs/1805.06907
Type Ia supernovae have two physical width-luminosity relations and they favor sub-Chandrasekhar and direct collision models – II. Color evolution
https://arxiv.org/abs/1805.06974
On the Nature of Long-Period Dwarf Novae with Rare and Low-Amplitude Outbursts
https://arxiv.org/abs/1805.07065
Discovery of deep eclipses in the cataclysmic variable IPHAS J051814.33+294113.0
https://arxiv.org/abs/1805.07073
Which evolutionary status does the Blue Large-Amplitude Pulsators stay at?
https://arxiv.org/abs/1805.07100
KIC 3240411 – the hottest known SPB star with the asymptotic g-mode period spacing
https://arxiv.org/abs/1805.07268
Models for Type Ia supernovae and related astrophysical transients
CS
Andreas
http://www.barchfeld.eu
PGP-Fingerprint: 1E72 BFA1 0B12 168B 2DE0 9508 116E F5E9 DD86 77B1
Variable Stars 