activity
20052025
most citedA CH3CN and HCO+ survey towards southern methanol masers associated with star formation

140 citations · 912 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.GA2025★ 6 cited

Non-thermal Radio Emission from Massive Protostars in the SARAO MeerKAT Galactic Plane Survey

W. O Obonyo, M. G Hoare, S. L Lumsden +7

We present an investigation of the L-band emission from known massive young stellar objects (MYSOs) in the SARAO MeerKAT Galactic Plane Survey to search for non-thermal radio emitt…

astro-ph.GA2025

High-resolution radio observations of massive protostars in the SARAO MeerKAT Galactic Plane Survey

W. O Obonyo, M. G Hoare, S. L Lumsden +2

We present high-resolution observations made with the Australia Telescope Compact Array (ATCA) at 5.5 GHz and 9.0 GHz of a sample of twenty-eight massive protostars. These protosta…

astro-ph.SR2023

The RMS survey: a census of massive YSO multiplicity in the -band

Robert G. Shenton, Rebecca J. Houghton, René D. Oudmaijer +4

Close to 100 per cent of massive stars are thought to be in binary systems. The multiplicity of massive stars seems to be intrinsically linked to their formation and evolution, and…

astro-ph.GA2023

Tracing Evolution in Massive Protostellar Objects (TEMPO) -- I: Fragmentation and emission properties of massive star-forming clumps in a luminosity limited ALMA sample

A. Avison, G. A. Fuller, N. Asabre Frimpong +16

The role of massive ( 8M) stars in defining the energy budget and chemical enrichment of the interstellar medium in their host galaxy is significant. In this first…

astro-ph.GA2023★ 25 cited

Kinematics and stability of high-mass protostellar disk candidates at sub-arcsecond resolution -- Insights from the IRAM NOEMA large program CORE

Aida Ahmadi, H. Beuther, F. Bosco +28

The fragmentation mode of high-mass molecular clumps and the accretion processes that form the most massive stars () are still not well understood. To this end,…

astro-ph.SR2022★ 1 cited

First spatially resolved Na I and He I transitions towards an MYSO. Finding new tracers for the gaseous star/disc interface

Evgenia Koumpia, M. Koutoulaki, W. -J. de Wit +4

With steady observational advances, the formation of massive stars is being understood in more detail. Numerical models are converging on a scenario where accretion discs play a ke…