most citedGas phase Elemental abundances in Molecular cloudS (GEMS) VII. Sulfur elemental abundance

73 citations

33 papers

astro-ph.EP2023★ 4 cited

Characterisation of chaos in meteoroid streams. Application to the Geminids

Ariane Courtot, Jérémie Vaubaillon, Marc Fouchard

Dynamically linking a meteor shower with its parent body can be challenging. This is in part due to the limits of the tools available today (such as D-criteria) but is also due to…

astro-ph.GA2023★ 29 cited

Multi-phase gas interactions on subarcsec scales in the shocked IGM of Stephan's Quintet with JWST and ALMA

P. N. Appleton, P. Guillard, B. Emonts +12

We combine JWST and HST imaging with ALMA~CO(2-1) spectroscopy to study the highly turbulent multi-phase intergalactic medium (IGM) in Stephan's Quintet on 25-150 pc scales. Previo…

astro-ph.GA2022★ 73 cited

Gas phase Elemental abundances in Molecular cloudS (GEMS) VII. Sulfur elemental abundance

A. Fuente, P. Rivière-Marichalar, L. Beitia-Antero +18

Gas phase Elemental abundances in molecular CloudS (GEMS) is an IRAM 30m large program aimed at determining the elemental abundances of carbon (C), oxygen (O), nitrogen (N), and su…

astro-ph.CO2022★ 5 cited

Non-local contribution from small scales in galaxy-galaxy lensing: Comparison of mitigation schemes

J. Prat, G. Zacharegkas, Y. Park +112

Recent cosmological analyses with large-scale structure and weak lensing measurements, usually referred to as 32pt, had to discard a lot of signal-to-noise from small scale…

astro-ph.GA2022★ 31 cited

Timing the r-Process Enrichment of the Ultra-Faint Dwarf Galaxy Reticulum II

Joshua D. Simon, Thomas M. Brown, Burçin Mutlu-Pakdil +65

The ultra-faint dwarf galaxy Reticulum II (Ret II) exhibits a unique chemical evolution history, with 72 +10/-12% of its stars strongly enhanced in r-process elements. We present d…

astro-ph.SR2022★ 5 cited

V838 Mon: A slow waking up of Sleeping Beauty?

T. Liimets, I. Kolka, M. Kraus +15

Context. V838 Monocerotis is a peculiar binary that underwent an immense stellar explosion in 2002, leaving behind an expanding cool supergiant and a hot B3V companion. Five years…