activity
20022026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 8.3k across the 160 of their papers we have counts for

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Showing astro-ph.GAShow all

14 papers · 1 filter

astro-ph.GA2025

Testing stellar yield prescriptions in OMEGA+: Implications for rising sodium abundances in young thick disc stars

Evans K. Owusu, Ashley J. Ruiter, Alex J. Kemp +8

We recently identified an upturn in [Na/Fe] for the population of Solar-type stars in the Galactic young thick disc () at super-Solar metallicity in…

astro-ph.GA2024

At the same age, metallicity, and alpha-enhancement, sodium is a more effective tracer of the young and old sequences of the Milky Way disc

Evans K. Owusu, Sven Buder, Ashley J. Ruiter +2

Trends in the enrichment of elements with stellar ages are a powerful avenue to identify unexplained origins of the elements. We investigate the stellar abundance trends of low to…

astro-ph.GA2022★ 9 cited

Evidence for a Dense, Inhomogeneous Circumstellar Medium in the Type Ia SNR 0519-69.0

Brian J. Williams, Parviz Ghavamian, Ivo R. Seitenzahl +3

We perform an expansion study of the Balmer dominated outer shock of the SNR 051969.0 in the LMC by using a combination of new HST WFC3 imagery obtained in 2020 and archival ACS…

astro-ph.GA2022★ 23 cited

Observational constraints on the origin of the elements. V. Non-LTE abundance ratios of [Ni/Fe] in Galactic stars and enrichment by sub-Chandrasekhar mass SNe

P. Eitner, M. Bergemann, A. J. Ruiter +4

We constrain the role of different SN Ia channels in the chemical enrichment of the Galaxy by studying the abundances of nickel in Galactic stars. We investigate four different SN…

astro-ph.GA2021★ 24 cited

First extragalactic measurement of the turbulence driving parameter: ALMA observations of the star-forming region N159E in the Large Magellanic Cloud

Piyush Sharda, Shyam H. Menon, Christoph Federrath +13

Studying the driving modes of turbulence is important for characterizing the impact of turbulence in various astrophysical environments. The driving mode of turbulence is parameter…

astro-ph.GA2020★ 8 cited

Imagery and UV Spectroscopy of the LMC Supernova Remnant N103B Using HST

William P. Blair, Parviz Ghavamian, John C. Raymond +6

We present HST/WFC3 multiband imagery of N103B, the remnant of a Type Ia supernova in the Large Magellanic Cloud, as well as HST/COS ultraviolet spectroscopy of the brightest radia…