718 citations · 6.7k across the 127 of their papers we have counts for
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Spatially resolved CIII]1909 emission in Haro 11
Genoveva Micheva, Göran Östlin, Jens Melinder +7
The CIII]1909 (hereafter, C III]) line is the strongest ultraviolet emission line after Ly and is therefore of interest to high redshift studies of star-forming (SF) galaxies ne…
Runaway OB Stars in the Small Magellanic Cloud: Dynamical Versus Supernova Ejections
J. Dorigo Jones, M. S. Oey, K. Paggeot +2
Runaway OB stars are ejected from their parent clusters via two mechanisms, both involving multiple stars: the dynamical ejection scenario (DES) and the binary supernova scenario (…
A Search for In-Situ Field OB Star Formation in the Small Magellanic Cloud
Irene Vargas-Salazar, M. S. Oey, Jesse R. Barnes +4
Whether any OB stars form in isolation is a question central to theories of massive star formation. To address this, we search for tiny, sparse clusters around 210 field OB stars f…
Size distribution of superbubbles
Biman B Nath, Pushpita Das, M. S. Oey
We consider the size distribution of superbubbles in a star forming galaxy. Previous studies have tried to explain the distribution by using adiabatic self-similar evolution of win…
Accretion-Driven Sources in Spatially Resolved Ly Emitters
B. Dittenber, M. S. Oey, E. Hodges-Kluck +4
Ly emission is a standard tracer of starburst galaxies at high redshift. However, a number of local Ly emitters (LAEs) are X-ray sources, suggesting a possible origin of Ly$α…