output
20162026
most citedGravitational waves from a first order electroweak phase transition: a brief review

178 citations

Showing astro-ph.SRShow all

15 papers · 1 filter

astro-ph.SR2026

White dwarf + M dwarf Detached Binaries in Long Period Radio Transients: Observed Binary Parameters, Evolution, and Population Constraints

Antonio C. Rodriguez, Kareem El-Badry, Iris de Ruiter +4

Long period radio transients (LPTs) are the slowest radio-pulsing sources ever found, with the current population spanning periods of seven minutes to over six hours. Two of the th…

astro-ph.SR2026

The neighboring stars of N6946-BH1 and the observational characteristics of failed supernovae

R. Forés-Toribio, C. S. Kochanek

Stellar collapse models predict that some stars more massive than 15 may collapse directly to a black hole, sometimes with a weak optical transient, a phenomenon kno…

astro-ph.SR2026

Closed-Form Statistical Relations Between Projected Separation, Semimajor Axis, Companion Mass, and Host Acceleration

Timothy D Brandt

I derive the statistical relationship between a radial velocity or astrometric acceleration (a trend), a companion's mass, and the projected separation of the companion. These rela…

astro-ph.SR2025

Vision-Based CNN Prediction of Sunspot Numbers from SDO/HMI Images

Fabian C. Quintero-Pareja, Diederik A. Montano-Burbano, Santiago Quintero-Pareja +1

Sunspot numbers provide the longest continuous record of solar activity and remain a key index for heliophysical research and space-weather applications. Standard sunspot determina…

astro-ph.SR2025★ 4 cited

Complex spectral variability and hints of a luminous companion in the Be star + black hole binary candidate ALS 8814

Kareem El-Badry, Matthias Fabry, Hugues Sana +2

The emission-line binary ALS 8814 was recently proposed as a Be star + black hole (BH) binary based on large-amplitude radial velocity (RV) variations of a Be star and non-detectio…

astro-ph.SR2025★ 3 cited

ASASSN-24fw: An 8-month long, 4.1 mag, optically achromatic and polarized dimming event

R. Forés-Toribio, B. JoHantgen, C. S. Kochanek +20

We discuss ASASSN-24fw, a 13th-magnitude star that optically faded by mag starting in September 2024 after over a decade of quiescence in ASAS-SN. The dimmimg…