output
20062026
most citedThe Effect of Starburst Metallicity on Bright X-Ray Binary Formation Pathways

163 citations

Showing 2023Show all

9 papers · 1 filter

q-bio.PE2023★ 7 cited

Modeling human activity-related spread of the spotted lanternfly (Lycorma delicatula) in the US

Daniel Strömbom, Autumn Sands, Jason M. Graham +4

The spotted lanternfly (Lycorma delicatula) has recently spread from its native range to several other countries and forecasts predict that it may become a global invasive pest. In…

astro-ph.SR2023★ 8 cited

Modeling Magnetically Channeled Winds in 3D: I. Isothermal Simulations of a Magnetic O Supergiant

Sethupathy Subramanian, Dinshaw S. Balsara, Asif ud-Doula +1

In this paper we present the first set of 3D magnetohydrodynamic (MHD) simulations performed with the riemann geomesh code. We study the dynamics of the magnetically channeled wind…

astro-ph.SR2023★ 61 cited

X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description

Jorick S. Vink, A. Mehner, P. A. Crowther +78

Observations of individual massive stars, super-luminous supernovae, gamma-ray bursts, and gravitational-wave events involving spectacular black-hole mergers, indicate that the low…

astro-ph.HE2023★ 6 cited

Discovery of extraordinary X-ray emission from magnetospheric interaction in the unique binary stellar system Lupi

B. Das, V. Petit, Y. Nazé +12

We report detailed X-ray observations of the unique binary system Lupi, the only known short-period binary consisting of two magnetic early-type stars. The components have comp…

astro-ph.SR2023★ 41 cited

X-Shooting ULLYSES: Massive stars at low metallicity. III. Terminal wind speeds of ULLYSES massive stars

C. Hawcroft, H. Sana, L. Mahy +26

The winds of massive stars have an impact on stellar evolution and on the surrounding medium. The maximum speed reached by these outflows, the terminal wind speed, is a global wind…

astro-ph.SR2023★ 5 cited

Seismological Studies of Pulsating DA White Dwarfs Observed with the Kepler Space Telescope and K2 Campaigns 1-8

Weston Hall, Barbara G. Castanheira, Agnès Bischoff-Kim

All single stars that are born with masses up to 8.5 - 10 will end their lives as a white dwarf (WD) star. In this evolutionary stage, WDs enter the cooling sequence, whe…