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20112023
most citedUnexpectedly large mass loss during the thermal pulse cycle of the red giant R Sculptoris!

192 citations · 1.4k across the 39 of their papers we have counts for

collaborators

39 papers

astro-ph.SR2023

The messy death of a multiple star system and the resulting planetary nebula as observed by JWST

Orsola De Marco, Muhammad Akashi, Stavros Akras +66

Planetary nebulae (PNe), the ejected envelopes of red giant stars, provide us with a history of the last, mass-losing phases of 90 percent of stars initially more massive than the…

astro-ph.HE2022★ 9 cited

Radio detections of IR-selected runaway stellar bow shocks

J. Van den Eijnden, P. Saikia, S. Mohamed

Massive stars moving at supersonic peculiar velocities through the interstellar medium (ISM) can create bow shocks, arc-like structures at the interface between the stellar wind an…

astro-ph.SR2022

3D models of the circumstellar environments of evolved stars: Formation of multiple spiral structures

Elias Aydi, Shazrene Mohamed

We present 3D hydrodynamic models of the interaction between the outflows of evolved, pulsating, Asymptotic Giant Branch (AGB) stars and nearby ( stellar radii) sub-stellar co…

astro-ph.GA2021★ 8 cited

L-GALAXIES 2020: The formation and chemical evolution of stellar haloes in Milky Way Analogues and galaxy clusters

Geoff G. Murphy, Robert M. Yates, Shazrene Mohamed

We present an analysis of the formation and chemical evolution of stellar haloes around (a) Milky Way Analogue (MWA) galaxies and (b) galaxy clusters in the L-Galaxies 2020 semi-an…

astro-ph.HE2021★ 15 cited

MeerKAT discovery of radio emission from the Vela X-1 bow shock

J. van den Eijnden, I. Heywood, R. Fender +7

Vela X-1 is a runaway X-ray binary system hosting a massive donor star, whose strong stellar wind creates a bow shock as it interacts with the interstellar medium. This bow shock h…

astro-ph.SR2021★ 13 cited

The binary central star of the bipolar pre-planetary nebula IRAS 08005-2356 (V510 Pup)

Rajeev Manick, Brent Miszalski, Devika Kamath +5

Current models predict that binary interactions are a major ingredient for the formation of bipolar planetary nebulae (PNe) and pre-planetary nebulae (PPNe). Despite years of radia…