astro-ph vom 2018-10-05

Moin,

https://arxiv.org/abs/1810.01892
Very high energy particle acceleration powered by the jets of the microquasar SS 433 (Anm.: SS 433 = V1343 Aql)

https://arxiv.org/abs/1810.02084
The W UMa binaries USNO-A2.0 1350-17365531, V471 Cas, V479 Lac and V560 Lac: light curve solutions and global parameters based on the GAIA distances

https://arxiv.org/abs/1810.02131
Rotation curve of the Milky Way from Classical Cepheids

https://arxiv.org/abs/1810.02154
Non-synchronous rotations in massive binary systems. HD93343 revisited

https://arxiv.org/abs/1810.02341
HD 202772A B: A Transiting Hot Jupiter Around A Bright, Mildly Evolved Star In A Visual Binary Discovered By Tess

CS
Andreas

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

Advertisements

astro-ph vom 2018-10-04

Moin,

https://arxiv.org/abs/1810.01465
Evidence for conservative mass transfer in the classical Algol system δ Librae from its surface carbon-to-nitrogen abundance ratio

https://arxiv.org/abs/1810.01472
An Optical Study of Two VY Sculptoris-Type Cataclysmic Binary Stars: V704 And and RX J2338+431

https://arxiv.org/abs/1810.01617
A near infrared variable star survey in the Magellanic Clouds: The Small Magellanic Cloud data

https://arxiv.org/abs/1810.01830
Impact of binary interaction on the evolution of blue supergiants

https://arxiv.org/abs/1810.01842
Orbital propeprties of binary post-AGB stars

CS
Andreas

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

astro-ph vom 2018-10-03

Moin,

https://arxiv.org/abs/1810.00922
Extended Optical/NIR Observations of Type Iax Supernova 2014dt: Possible Signatures of a Bound Remnant

https://arxiv.org/abs/1810.00982
Fates of the oldest intermediate-mass stars – Primordial to Extremely Metal-Poor AGB and Super-AGB Stars: White Dwarf or Supernova progenitors

https://arxiv.org/abs/1810.01025
Impacts of the New Carbon Fusion Cross Sections on Type Ia Supernovae

https://arxiv.org/abs/1810.01149
Investigating the Unusual Spectroscopic Time-Evolution in SN b2012fr

https://arxiv.org/abs/1810.01204
The loud and the quiet: searching for radio counterparts of two radio-weak BL Lac candidates with VLBI

https://arxiv.org/abs/1810.01287
Testing the speed of light over cosmological distances: the combination of strongly lensed and unlensed supernova Ia

CS
Andreas

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

astro-ph vom 2018-10-02

Moin,

https://arxiv.org/abs/1810.00006
An Improved Orbital Period for GY Cancri Based on Two K2 Campaigns

https://arxiv.org/abs/1810.00011
The Relative Specific Type Ia Supernovae Rate From Three Years of ASAS-SN

https://arxiv.org/abs/1810.00334
A Linear and Quadratic Time-Frequency Analysis of Gravitational Waves from Core-Collapse Supernovae

CS
Andreas

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

astro-ph vom 2018-10-01

Moin,

https://arxiv.org/abs/1809.10812
Constraining small scale magnetic fields through plasma lensing: Application to the Black widow eclipsing pulsar binary (Anm.: PSR B1957+20 = QX Sge)

https://arxiv.org/abs/1809.11032
Maximally dusty star-forming galaxies: Supernova dust production and recycling in Local Group and high-redshift galaxies

https://arxiv.org/abs/1809.11145
The Photometric LSST Astronomical Time-series Classification Challenge (PLAsTiCC): Selection of a performance metric for classification probabilities balancing diverse science goals

CS
Andreas

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

astro-ph vom 2018-09-28

Moin,

https://arxiv.org/abs/1809.10146
Three-Dimensional Core-Collapse Supernova Simulations with Multi-Dimensional Neutrino Transport Compared to the Ray-by-Ray-plus Approximation

https://arxiv.org/abs/1809.10147
Rates and Properties of Strongly Gravitationally Lensed Supernovae and their Host Galaxies in Time-Domain Imaging Surveys

https://arxiv.org/abs/1809.10157
Understanding the orbital periods of CEMP-s stars
(Anm.: “ The chemical enrichments detected in CEMP-s stars are believed to be the consequence of a mass-transfer episode from a now extinct AGB primary star. This hypothesis is borne out by the fact that most CEMP-s stars exhibit RV variations suggesting that they are in binary systems. … With a set of default assumptions often made in binary population-synthesis studies, the percentage of observed CEMP-s systems with periods shorter than 2000 days is underestimated by almost a factor of 3, and by a factor of 2 between 3000 and 10000 days, while 40% of the simulated systems have periods longer than 10000 days, which is approximately the longest measured period among CEMP-s stars.“)

https://arxiv.org/abs/1809.10187
Three Dimensional Radiation Hydrodynamic Simulations of Massive Star Envelopes
(ANm.: „… While in outburst, most LBVs stay on the cold S Dor instability strip …“)

https://arxiv.org/abs/1809.10376
Multiple Star Systems in the Orion Nebula

CS
Andreas

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

astro-ph vom 2018-09-27

Moin,

https://arxiv.org/abs/1809.09623
Spectroscopic binaries among AGB stars from HERMES/Mercator: the case of V Hya

https://arxiv.org/abs/1809.09628
ASAS-SN Identification of FY Sct as a detached eclipsing binary system with a ~2.6 year period

https://arxiv.org/abs/1809.10065
Constraining the nature of DG Tau A’s thermal and non-thermal radio emission

https://arxiv.org/abs/1809.10071
Binary Red Supergiants: A New Method for Detecting B-type Companions

https://arxiv.org/abs/1809.10077
Asymptotic Giant Branch Variables in Nearby Galaxies

CS
Andreas

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

astro-ph vom 2018-09-26

Moin,

https://arxiv.org/abs/1809.09103
Helium giant stars as progenitors of rapidly fading Type Ibc supernovae

https://arxiv.org/abs/1809.09150
The impact of pre-white dwarf evolution on the pulsational properties and asteroseismological inferences of ZZ Ceti stars

https://arxiv.org/abs/1809.09242
Evolution and Asteroseismology of Pulsating Low-Mass White Dwarfs

https://arxiv.org/abs/1809.09447
A magnetic study of the δ Scuti variable HD 21190 and the close solar-type background star CPD -83∘ 64B

https://arxiv.org/abs/1809.09451
New Photometric Pipeline to Explore Temporal and Spatial Variability with KMTNet DEEP-South Observations

CS
Andreas

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

astro-ph vom 2018-09-25

Moin,

https://arxiv.org/abs/1809.08398
Charged-current scattering off 16O nucleus as a detection channel for supernova neutrinos

https://arxiv.org/abs/1809.08741
Origin of magnetic fields in cataclysmic variables

https://arxiv.org/abs/1809.09015
An XMM-Newton observation of the symbiotic star AG Peg: the X-ray emission after the end of its 2015 outburst

https://arxiv.org/abs/1809.09055
A decade of dust formation in the Type IIn SN 2005ip

CS
Andreas

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