activity
20062023
most citedV1309 Scorpii: merger of a contact binary

482 citations · 1.1k across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.SR2023

The heart of Sakurai's Object revealed by ALMA

Daniel Tafoya, Peter A. M. van Hoof, Jesus A. Toala +7

We present high angular-resolution observations of Sakurai's object using the Atacama Large Millimeter Array, shedding new light on its morpho-kinematical structure. The millimetre…

astro-ph.GA2022★ 39 cited

V-LoTSS: The Circularly-Polarised LOFAR Two-metre Sky Survey

J. R. Callingham, T. W. Shimwell, H. K. Vedantham +44

We present the detection of 68 sources from the most sensitive radio survey in circular polarisation conducted to date. We use the second data release of the 144 MHz LOFAR Two-metr…

astro-ph.SR2022★ 3 cited

Recombination of hot ionized nebulae: The old planetary nebula around V4334 Sgr (Sakurai's star)

Martin Reichel, Stefan Kimeswenger, Peter A. M. van Hoof +5

After becoming ionized, low-density astrophysical plasmas will begin a process of slow recombination. Models for this still have significant uncertainties. The recombination cannot…

astro-ph.SR2022★ 14 cited

Lithium in coalesced non-compact stars

Tomek Kamiński, Mirek Schmidt, Marcin Hajduk +3

Context. Galactic red novae are thought to be produced in stellar mergers between non-compact stars, such as main-sequence stars and cool giants. They are hoped to help in explaini…

astro-ph.SR2022★ 21 cited

Peculiar radioX-ray relationship in active stars

H. K. Vedantham, J. R. Callingham, T. W. Shimwell +5

The empirical relationship between the non-thermal 5GHz radio luminosity and the soft X-ray luminosity of active stellar coronae, canonically called the Güdel-Benz relationship (Gü…

astro-ph.SR2021

Evidence for cold plasma in planetary nebulae from radio observations with the LOw Frequency ARray (LOFAR)

Marcin Hajduk, Marijke Haverkorn, Timothy Shimwell +6

We present observations of planetary nebulae with the LOw Frequency ARray (LOFAR) between 120 and 168 MHz. The images show thermal free-free emission from the nebular shells. We ha…