activity
20032026
most citedThe GALAH Survey: Scientific Motivation

839 citations · 2.7k across the 49 of their papers we have counts for

collaborators

50 papers

astro-ph.SR2026

Structure of Convective-Reactive Zone in a Supernova Progenitor

M. Mocak, C. Meakin, F. Rizzuti +5

Convective-reactive events are phases of stellar evolution where turbulent mixing and nuclear burning directly compete, since their timescales become similar within convection zone…

astro-ph.SR2024

Structural and Nucleosynthetic Evolution of Metal-poor & Metal-free Low- and Intermediate-Mass Stars

Simon Wattana Campbell

In this PhD thesis we investigate stellar evolution and nucleosynthesis in the low- and extremely-low metallicity regime - including models of stars with a pure Big Bang compositio…

astro-ph.GA2024★ 20 cited

The GALAH survey: Tracing the Milky Way's formation and evolution through RR Lyrae stars

Valentina D'Orazi, Nicholas Storm, Andrew R. Casey +39

Stellar mergers and accretion events have been crucial in shaping the evolution of the Milky Way (MW). These events have been dynamically identified and chemically characterised us…

astro-ph.SR2023

Asteroseismology sheds light on the origin of carbon-deficient red giants: likely merger products and linked to the Li-rich giants

Sunayana Maben, Simon W. Campbell, Yerra Bharat Kumar +2

Carbon-deficient red giants (CDGs) are a peculiar class of stars that have eluded explanation for decades. We aim to better characterise CDGs by using asteroseismology (Kepler, TES…

astro-ph.GA2023

A large sample of newly-identified carbon-deficient red giants from APOGEE

Sunayana Maben, Yerra Bharat Kumar, Bacham E. Reddy +2

Based on the APOGEE survey we conducted a search for carbon-deficient red giants (CDGs). We found 103 new CDGs, increasing the number in the literature by more than a factor of 3.…

astro-ph.SR2023★ 1 cited

First Asteroseismic Analysis of the Globular Cluster M80: Multiple Populations and Stellar Mass Loss

Madeline Howell, Simon W. Campbell, Dennis Stello +1

Asteroseismology provides a new avenue for accurately measuring the masses of evolved globular cluster (GC) stars through the detection of their solar-like oscillations. We present…