11 citations · 18 across the 5 of their papers we have counts for
5 papers
A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk
Olivier Berné, Emilie Habart, Els Peeters +143
Most low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict that this FUV radiati…
METAL-Z: Measuring dust depletion in low metalicity dwarf galaxies
Aleksandra Hamanowicz, Kirill Tchernyshyov, Julia Roman-Duval +6
The cycling of metals between interstellar gas and dust is a critical aspect of the baryon cycle of galaxies, yet our understanding of this process is limited. This study focuses o…
Dust around massive stars is agnostic to galactic environment: New insights from PHAT/BEAST
Christina Willecke Lindberg, Claire Murray, Julianne Dalcanton +2
Resolving the environments of massive stars is crucial for understanding their formation mechanisms and their impact on galaxy evolution. An important open question is whether mass…
Metal Abundances and Depletions in the Neutral Interstellar Medium of Galaxies: the Local Volume as a Laboratory
Julia Roman-Duval, Alessandra Aloisi, Karl Gordon +8
The comparison of chemical abundances in the neutral gas of galaxies to photospheric abundances of old and young stars, ionized gas abundances, and abundances in galactic halos can…
A new method for deriving the stellar birth function of resolved stellar populations
Mario Gennaro, Kirill Tchernyshyov, Tom Brown +1
We present a new method for deriving the stellar birth function (SBF) of resolved stellar populations. The SBF (stars born per unit mass, time, and metallicity) is the combination…