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Optical Multi-Channel Intensity Interferometry - or: How To Resolve O-Stars in the Magellanic Clouds
Sascha Trippe, Jae-Young Kim, Bangwon Lee +6
Intensity interferometry, based on the Hanbury Brown-Twiss effect, is a simple and inexpensive method for optical interferometry at microarcsecond angular resolutions; its use in a…
UKIRT Widefield Infrared Survey for Fe
Jae-Joon Lee, Bon-Chul Koo, Yong-Hyun Lee +17
The United Kingdom Infrared Telescope (UKIRT) Widefield Infrared Survey for Fe (UWIFE) is a 180 deg imaging survey of the first Galactic quadrant (7 < l < 62$^{\c…
Explosion and nucleosynthesis of low redshift pair instability supernovae
Alexandra Kozyreva, Sung-Chul Yoon, Norbert Langer
Both recent observations and stellar evolution models suggest that pair-instability supernovae (PISNe) could occur in the local Universe, at metallicities below Z_Sun/3. Previous P…
Dust Production Factories in the Early Universe: Formation of Carbon Grains in Red-supergiant Winds of Very Massive Population III Stars
Takaya Nozawa, Sung-Chul Yoon, Keiichi Maeda +3
We investigate the formation of dust in a stellar wind during the red-supergiant (RSG) phase of a very massive Population III star with the zero-age main sequence mass of 500 M_sun…