output
19982026
most citedRotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones

888 citations

Showing 2019Show all

51 papers · 1 filter

astro-ph.SR2019★ 67 cited

The Tarantula Massive Binary Monitoring: III. Atmosphere analysis of double-lined spectroscopic systems

L. Mahy, H. Sana, M. Abdul-Masih +17

Accurate stellar parameters of individual objects in binary systems are essential to constrain the effects of binarity on stellar evolution. These parameters serve as a prerequisit…

astro-ph.SR2019★ 35 cited

Pulsation in faint blue stars

Conor M. Byrne, C. Simon Jeffery

Following the discovery of blue large-amplitude pulsators (BLAPs) by the OGLE survey, additional hot, high-amplitude pulsating stars have been discovered by the Zwicky Transient Fa…

astro-ph.SR2019★ 29 cited

Observations and 3D MHD Modeling of a Confined Helical Jet Launched by a Filament Eruption

Lauren Doyle, Peter F. Wyper, Eamon Scullion +3

We present a detailed analysis of a confined filament eruption and jet associated with a C1.5 class solar flare. Multi-wavelength observations from GONG and SDO reveal the filament…

astro-ph.GA2019★ 32 cited

Radio Observations of Supernova Remnant G1.9+0.3

Kieran J. Luken, Miroslav D. Filipović, Nigel I. Maxted +18

We present 1 to 10GHz radio continuum flux density, spectral index, polarisation and Rotation Measure (RM) images of the youngest known Galactic Supernova Remnant (SNR) G1.9+0.3, u…

astro-ph.SR2019★ 109 cited

Properties of OB star-black hole systems derived from detailed binary evolution models

N. Langer, C. Schürmann, K. Stoll +38

The recent gravitational wave measurements have demonstrated the existence of stellar mass black hole binaries. It is essential for our understanding of massive star evolution to i…

astro-ph.SR2019★ 5 cited

No evidence of a sudden change of spectral appearance or magnetic field strength of the O9.7V star HD 54879

G. A. Wade, S. Bagnulo, Z. Keszthelyi +8

It was recently claimed that the magnetic O-type star HD 54879 exhibits important radial velocity variability indicative of its presence in a spectroscopic binary. More remarkably,…