activity
20242026
collaborators

8 papers

astro-ph.SR2026

Wind Accretion in Massive Binaries Experiencing High Mass Loss Rates: II. Eccentricity

Bhawna Mukhija, Amit Kashi

We perform numerical simulations to investigate high-power wind accretion in massive binary systems undergoing enhanced mass-loss episodes. The primary star is taken in the mass ra…

astro-ph.SR2026

Envelope Inflation and outflow Driven by Energy Deposition in Massive Stars

Bhawna Mukhija, Amit Kashi

Evolved massive stars are known to undergo outflow with high mass ejections, resulting in the loss of a substantial portion of their envelopes. One proposed mechanism driving these…

astro-ph.SR2025

Pre-Supernova Multiple Giant Eruptions in Massive Stars

Bhawna Mukhija, Amit Kashi

Massive stars can exhibit giant eruptions with high mass loss shortly before their explosion as a core-collapse Supernova. These multiple giant eruptions (MGEs) may have a commutat…

astro-ph.SR2025

Effect of gravity darkening and oblate factor in rapidly rotating massive stars

Bhawna Mukhija, Michel Curé, Ignacio Araya +2

Context. Rapid rotation in massive stars leads to gravity darkening and oblateness, significantly affecting their radiation-driven winds. These effects can alter wind dynamics and…

astro-ph.SR2025

Wind Accretion in Massive Binaries Experiencing High Mass Loss Rates: I. Dependency on Mass Ratio and Orbital Period

Bhawna Mukhija, Amit Kashi

We run numerical simulations to study high-power wind accretion in a massive binary system during a high mass loss event. The system consists of an evolved primary star with a zero…

astro-ph.SR2025

High Power Accretion in Massive Binary Systems and the Impact of Metallicity

Bhawna Mukhija, Amit Kashi

During a giant eruption of a very massive star in the binary system, the companion star can accrete a large amount of mass that can change its properties and potentially its subseq…