astro-ph vom 2019-01-07

Moin,

https://arxiv.org/abs/1901.00871
The SPIRITS sample of Luminous Infrared Transients: Uncovering Hidden Supernovae and Dusty Stellar Outbursts in Nearby Galaxies

https://arxiv.org/abs/1901.00872
Host Galaxies of Type Ic and Broad-lined Type Ic Supernovae from the Palomar Transient Factory: Implication for Jet Production

https://arxiv.org/abs/1901.00874
ZTF 18aaqeasu (SN 2018byg): A Massive Helium-shell Double Detonation on a Sub-Chandrasekhar Mass White Dwarf

https://arxiv.org/abs/1901.00903
Flat Spectrum Radio Continuum Emission Associated with ε Eridani

https://arxiv.org/abs/1901.00974
The morpho-kinematics of the circumstellar envelope around the AGB star EP Aqr

https://arxiv.org/abs/1901.01197
Observational Constraints on Late-Time Radio Rebrightening of GRB-Supernovae

CS
Andreas

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

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astro-ph vom 2019-01-04

Moin,

https://arxiv.org/abs/1901.00531
Distinguishing Circumstellar from Stellar Photometric Variability in Eta Carinae

https://arxiv.org/abs/1901.00778
Physics of Planet Trapping with Applications to HL Tau

https://arxiv.org/abs/1901.00821
Launching of hot gas outflow by disc-wide supernova explosions

CS
Andreas

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

astro-ph vom 2019-01-03

Moin,

https://arxiv.org/abs/1901.00009
The ASAS-SN Catalog of Variable Stars III: Variables in the Southern TESS Continuous Viewing Zone

https://arxiv.org/abs/1901.00030
NuSTAR Detection of X-rays Concurrent with Gamma Rays in the Nova V5855 Sgr

https://arxiv.org/abs/1901.00173
On the mass of supernova progenitors: the role of the 12C+12C reaction

https://arxiv.org/abs/1901.00237
Period variations and long-term cyclic changes in the light curve for the very short-period K-type contact binary YZ Phe

https://arxiv.org/abs/1901.00340
He-accreting WD: Nucleosynthesis in the extreme binary system (1.02+0.30) M⊙
(Anm.: „… Our results strongly suggest that massive AM CVn systems with WD donors do not experience a final very strong dynamical He-flash driving an explosive event like SN .Ia. …“)

https://arxiv.org/abs/1901.00404
Optical spectroscopic and polarization properties of 2011 outburst of the recurrent nova T Pyxidis

https://arxiv.org/abs/1901.00407
HIDES spectroscopy of bright detached eclipsing binaries from the Kepler field – III. Spectral analysis, updated parameters, and new systems

CS
Andreas

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

astro-ph vom 2019-01-01

Moin,

https://arxiv.org/abs/1812.11338
From Dinuclear Systems to Close Binary Stars: Application to Source of Energy in the Universe

https://arxiv.org/abs/1812.11432
Condensation of SiC Stardust in CO Nova Outbursts

https://arxiv.org/abs/1812.11435
On the magnetisation and the radiative efficiency of BL Lac jets

https://arxiv.org/abs/1812.11692
Detection of Circumstellar Helium in Type Iax Progenitor Systems

https://arxiv.org/abs/1812.11907
Exoplanets in the Antarctic Sky. I. The First Data Release of AST3-II (CHESPA) and New Found Variables within the Southern CVZ of TESS

CS
Andreas

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

astro-ph vom 2018-12-31

Moin,

https://arxiv.org/abs/1812.10492
Serendipitous Discoveries of Kilonovae in the LSST Main Survey: Maximising Detections of Sub-Threshold Gravitational Wave Events

https://arxiv.org/abs/1812.10871
Evolution of V339 Del (Nova Del 2013) since 0.37 to 75 Days after Discovery

https://arxiv.org/abs/1812.10874
Photometric Investigation of Novae T Pyx, BT Mon and V574 Pup at Quiescence by using the 2.4 m Thai National Telescope

https://arxiv.org/abs/1812.11083
Three-dimensional mixing and light curves: constraints on the progenitor of supernova 1987A

Ich wünsche Euch einen schönen Jahreswechsel und ein gesundes und erfolgreiches Jahr 2019.

CS
Andreas

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

astro-ph vom 2018-12-27

Moin,

https://arxiv.org/abs/1812.09535
Hen 3-160 – the first symbiotic binary with Mira variable S star

https://arxiv.org/abs/1812.09725
The Local Group Dwarf Galaxies: The Star Formation Histories derived using the Long Period Variable stars

https://arxiv.org/abs/1812.09786
Stress testing the dark energy equation of state imprint on supernova data

https://arxiv.org/abs/1812.09811
Comparing treatments of weak reactions with nuclei in simulations of core-collapse supernovae

https://arxiv.org/abs/1812.09856
Photometric Investigation of the Contact Binary GU Ori with High Metallicity

https://arxiv.org/abs/1812.09907
Accretion geometry of the black-hole binary Cygnus X-1 from X-ray polarimetry (Anm.: Cygnus X-1 = V1357 Cyg)

https://arxiv.org/abs/1812.09989
Multiplicity of Galactic Cepheids from long-baseline interferometry. IV. New detected companions from MIRC and PIONIER observations

https://arxiv.org/abs/1812.09993
HST FUV spectroscopy of the short orbital period recurrent nova CI Aql: Implications for white dwarf mass evolution

https://arxiv.org/abs/1812.10161
The Breakthrough Listen Search for Intelligent Life: Searching Boyajian’s Star for Laser Line Emission (Anm.: Boyajian’s Stern ist ein nicht einzuordnender Veränderlicher)

https://arxiv.org/abs/1812.10289
Ultrahigh-energy cosmic-ray nuclei and neutrinos from engine-driven supernovae

CS
Andreas

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

astro-ph vom 2018-12-24

Moin,

https://arxiv.org/abs/1812.08793
The long-term evolution and appearance of Type Iax postgenitor stars

https://arxiv.org/abs/1812.08799
Excluding super-soft X-ray sources as progenitors for four Type Ia supernovae in the Large Magellanic Cloud

https://arxiv.org/abs/1812.08811
Infrared Spectroscopy of Symbiotic Stars. XII. The Neutron Star SyXB System 4U 1700+24 = V934 Herculis

https://arxiv.org/abs/1812.09020
New light curve solution of V568 Peg and first determination of its fundamental parameters

Allen Lesern wünsche ich ein besinnliches Weihnachtsfest.

CS
Andreas

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

astro-ph vom 2018-12-21

Moin,

https://arxiv.org/abs/1812.08170
CI Camelopardalis: The first sgB[e]-High Mass X-ray Binary Twenty Years on, a Supernova Imposter in our own Galaxy?

https://arxiv.org/abs/1812.08175
Gas Flows Within Cavities of Circumbinary Discs in Eccentric Binary Protostellar Systems

https://arxiv.org/abs/1812.08230
Remnants and ejecta of thermonuclear electron-capture supernovae: Constraining oxygen-neon deflagrations in high-density white dwarfs

https://arxiv.org/abs/1812.08234
The Evolution of Dust Opacity in Core Collapse Supernovae and the Rapid Formation of Dust in Their Ejecta

https://arxiv.org/abs/1812.08695
Detecting the signatures of helium in type Iax supernovae

https://arxiv.org/abs/1812.08746
Ultraviolet Activity as indicator of Small-scale Magnetic Fields in gamma Cassiopeiae

Weihnachten bei arXiv:
December 2018 Holiday Schedule: The mailings and the public availability of new submissions will be deferred for 24 December, 25 December, and 27 December 2018, as well as 1 January 2019. The arXiv servers will otherwise remain in operation. In addition, arXiv staff will provide limited service in response to queries during these periods.

Articles received at or after 14:00 ET Thursday, 20 December 2018 and before 14:00 ET Friday, 21 December 2018 will be announced at 20:00 ET Sunday, 23 December 2018.
Articles received at or after 14:00 ET Friday, 21 December 2018 and before 14:00 ET Wednesday, 26 December 2018 will be announced at 20:00 ET Wednesday, 26 December 2018.
Articles received at or after 14:00 ET Wednesday, 26 December 2018 and before 14:00 ET Friday, 28 December 2018 will be announced at 20:00 ET Sunday, 30 December 2018.
Articles received at or after 14:00 ET Friday, 28 December 2018 and before 14:00 ET Monday, 31 December 2018 will be announced at 20:00 ET Monday, 31 December 2018.
Articles received at or after 14:00 ET Monday, 31 December 2018 and before 14:00 ET Wednesday, 2 January 2019 will be announced at 20:00 ET Wednesday, 2 January 2019.
Note: articles submitted at or after 14:00 ET Monday, 31 December 2018 will receive arXiv:1901.nnnnn identifiers.

CS
Andreas

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

astro-ph vom 2018-12-20

Moin,

https://arxiv.org/abs/1812.07569
FBOTs and AT2018cow following electron-capture collapse of merged white dwarfs

https://arxiv.org/abs/1812.07618
ALMA polarimetric studies of rotating jet/disk systems
(Anm.: „We have recently obtained polarimetric data at mm wavelengths with ALMA for the young systems DG Tau and CW Tau, …“)

https://arxiv.org/abs/1812.07620
Supernovae from blue supergiant progenitors: What a mess!

https://arxiv.org/abs/1812.07631
K2 Ultracool Dwarfs Survey. V. High superflare rates on rapidly rotating late-M dwarfs

https://arxiv.org/abs/1812.07703
Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae

https://arxiv.org/abs/1812.07796
Luminous AGB variables in the dwarf Irregular Galaxy, NGC 3109

https://arxiv.org/abs/1812.08070
Starspots in contact and semi-detached binary systems

CS
Andreas

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

astro-ph vom 2018-12-19

Moin,

https://arxiv.org/abs/1812.07175
The Evolution towards Electron-capture Supernovae: the Flame Propagation and the Pre-bounce Electron-neutrino Radiation

https://arxiv.org/abs/1812.07185
Semiregular variable stars

https://arxiv.org/abs/1812.07307
A crystal ball for kilonovae

https://arxiv.org/abs/1812.07404
Radio background and IGM heating due to Pop III supernovae explosions

https://arxiv.org/abs/1812.07434
The interplay between pulsation, mass loss, and third dredge-up: More about Miras with and without technetium

https://arxiv.org/abs/1812.07486
Spectral analysis of the extremely hot DA white dwarf PG0948+534
(Anm.: „… This is supported by the V-band variability that shows a period of P=3.45 d (amplitude 0.19 mag), which we interpret as the star’s rotation period. …“)

https://arxiv.org/abs/1812.07552
Ultralow-amplitude RR Lyrae Stars in M4

CS
Andreas

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