astro-ph vom 2017-11-07

Moin,

https://arxiv.org/abs/1711.01275
Observations of SN 2015F suggest a correlation between the intrinsic luminosity of Type Ia supernovae and the shape of their light curves >900 days after explosion

https://arxiv.org/abs/1711.01298
About ionization zones remaining after supernovae explosions

https://arxiv.org/abs/1711.01338
Probing the structure of Kepler ZZ Ceti stars with full evolutionary models-based asteroseismology

https://arxiv.org/abs/1711.01529
Recurrent novae and long-term evolution of mass-accreting white dwarfs — toward the accurate mass retention efficiency

https://arxiv.org/abs/1711.01534
Far-UV HST Spectroscopy of An Unusual Hydrogen Poor Superluminous Supernova: SN2017egm

https://arxiv.org/abs/1711.01564
Noise Sources in Photometry and Radial Velocities

https://arxiv.org/abs/1711.01727
An Estimation of the White Dwarf Mass in the Dwarf Nova GK Persei with NuSTAR Observations of Two States

https://arxiv.org/abs/1711.01749
Optical flickering of the symbiotic star CH Cyg

https://arxiv.org/abs/1711.01958
Discovery of radio emission from the symbiotic X-ray binary system GX 1+4 (Anm.: GX 1+4 = V2116 Oph)

https://arxiv.org/abs/1711.01959
An Introduction to Data Analysis in Asteroseismology

https://arxiv.org/abs/1711.02011
Evolution of post-Accretion Induced Collapse Binaries: the Effect of Evaporation

Archiv:
https://veraenderlichesterne.wordpress.com/

CS
Andreas

http://www.barchfeld.eu
PGP-Fingerprint: 1E72 BFA1 0B12 168B 2DE0 9508 116E F5E9 DD86 77B1

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