most citedEvaluating the impact of binary parameter uncertainty on stellar population properties

25 citations · 43 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202025 cited

Evaluating the impact of binary parameter uncertainty on stellar population properties

E. R. Stanway, A. A. Chrimes, J. J. Eldridge +2

Binary stars have been shown to have a substantial impact on the integrated light of stellar populations, particularly at low metallicity and early ages - conditions prevalent in t…

astro-ph.SR2020

A systematic aging method I: HII regions D118 and D119 in NGC 300

H. F. Stevance, J. J. Eldridge, A. McLeod +2

Accurately determining the age of H\,{ii} regions and the stars they host is as important as it is challenging. Historically the most popular method has been isochrone fitting to H…

astro-ph.SR2020

The shape of SN 1993J re-analyzed

H. F. Stevance, D. Baade, J. R. Bruten +8

SN 1993J is one of the best studied Type IIb supernovae. Spectropolarimetric data analyses were published over two decades ago at a time when the field of supernova spectropolarime…

astro-ph.SR2019

Weighing in on black hole binaries with BPASS: LB-1 does not contain a 70M black hole

J. J. Eldridge, E. R. Stanway, K. Breivik +3

The recent identification of a candidate very massive 70 M(Sun) black hole is at odds with our current understanding of stellar winds and pair-instability supernovae. We investigat…

astro-ph.HE2019

Linear spectropolarimetry of 35 Type Ia Supernovae with VLT/FORS: An analysis of the Si II line polarization

Aleksandar Cikota, Ferdinando Patat, Lifan Wang +9

Spectropolarimetry enables us to measure the geometry and chemical structure of the ejecta in supernova explosions, which is fundamental for the understanding of their explosion me…

astro-ph.SR20191 cited

Spectropolarimetry of stripped envelope core collapse supernovae and their progenitors

H. F. Stevance

Over the past 30 years, spectropolarimetry has proven to be a great tool to probe the 3D geometry of core collapse supernovae (CCSNe). The number of high-quality multi-epoch spectr…