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SUMMARY:Uncovering Extremely Metal-Poor Galaxies in the Era of JWST Studie
 s - Yuki Isobe (University of Tokyo)
DTSTART:20221007T103000Z
DTEND:20221007T113000Z
UID:TALK180428@talks.cam.ac.uk
CONTACT:Sandro Tacchella
DESCRIPTION:To prepare for JWST/NIRSpec deeper observations\, we have inve
 stigated chemical abundances and kinematics of local (z=0.01) extremely me
 tal-poor galaxies (EMPGs) as analogs of high-z primordial galaxies.\nOur c
 hemical enrichment models suggest that high Fe/O ratios of EMPGs (approx. 
 solar abundance) can be explained by supernovae originating from metal-poo
 r massive stars (> 30 Msun). Our Subaru IFU observations also show that EM
 PGs have rotational velocities (v_rot = 5-23 km s-1) lower than their velo
 city dispersions (σ = 17-31 km s-1)\, which suggests that high-z primordi
 al galaxies are also dispersion-dominated systems (i.e.\, v_rot/σ < 1).\n
LOCATION:in person &amp\; via zoom 
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