activity
20022026
most citedQuantifying the uncertainties of chemical evolution studies. II. Stellar yields

409 citations · 2.8k across the 44 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2024★ 1 cited

Nova contributions to the chemical evolution of the Milky Way

Alex J. Kemp, Amanda I. Karakas, Andrew R. Casey +3

Context. The explosive burning that drives nova eruptions results in unique nucleosynthesis that heavily over-produces certain isotopes relative to the solar abundance. However, no…

astro-ph.GA2020★ 117 cited

The GALAH survey: tracing the Galactic disk with Open Clusters

Lorenzo Spina, Yuan-Sen Ting, Gayandhi M. De Silva +28

Open clusters are unique tracers of the history of our own Galaxy's disk. According to our membership analysis based on \textit{Gaia} astrometry, out of the 226 potential clusters…

astro-ph.GA2018★ 28 cited

X-shooting GRBs at high redshift: probing dust production history

T. Zafar, P. Møller, D. Watson +16

Evolved asymptotic giant branch (AGB) stars and Type Ia supernovae (SNe) are important contributors to the elements that form dust in the interstellar medium of galaxies, in partic…

astro-ph.GA2013★ 4 cited

3He: Does the problem persists?

L. Guzman-Ramirez, J. E. Pineda, A. A. Zijlstra +2

To understand the chemical evolution of the Galaxy, we need to understand the contribution of PNe in the 3He abundance. 3He abundances have been detected only in a couple of PNe, t…

astro-ph.GA2011★ 1 cited

The curious conundrum regarding sulfur and oxygen abundances in planetary nebulae

R. B. C. Henry, A. Speck, A. I. Karakas +1

We carefully consider numerous explanations for the sulfur abundance anomaly in planetary nebulae. No one rationale appears to be satisfactory, and we suggest that the ultimate exp…

astro-ph.GA2010★ 409 cited

Quantifying the uncertainties of chemical evolution studies. II. Stellar yields

D. Romano, A. I. Karakas, M. Tosi +1

This is the second paper of a series which aims at quantifying the uncertainties in chemical evolution model predictions related to the underlying model assumptions. Specifically,…