Moin,
https://arxiv.org/abs/1807.10321
Optical observations of „hot“ novae returning to quiescence
https://arxiv.org/abs/1807.10391
The Ultraviolet Colors of Type Ia Supernovae and their Photospheric Velocities
https://arxiv.org/abs/1807.10506
Neutrino emission from BL Lac objects: the role of radiatively inefficient accretion flows
https://arxiv.org/abs/1807.10533
K2 observations of the rapidly oscillating Ap star 33 Lib (HD 137949): new frequencies and unique non-linear interactions
https://arxiv.org/abs/1807.10646
Two-dimensional simulations of mixing in classical novae: the effect of the white dwarf composition and mass
https://arxiv.org/abs/1807.10735
Candidate Wide-separation Companions to Nearby, Dusty Young Stars: Gaia Weighs In
(Anm.: „… For three of the proposed wide pairs — TW Hya + 2M1102-34; HR 4796A + 2M1235-39; and V4046 Sgr AB + GSC 07396 — the Gaia DR2 data confirm that the two stars lie at the same distance and are comoving (or nearly so), to within the measurement errors. …“)
OT:
https://arxiv.org/abs/1807.10593
How dark can it get at night? Examining how clouds darken the sky via all-sky differential photometry
CS
Andreas
http://www.barchfeld.eu
PGP-Fingerprint: 1E72 BFA1 0B12 168B 2DE0 9508 116E F5E9 DD86 77B1