Session 3.2: Origin and evolution, progenies and progenitors
Chair: Weikai Zong
› Hot Subdwarf Stars from LAMOST DR5 and Gaia DR2 - Zhanwen Han, Yunnan Observatories
09:00-09:20 (20min)
› Mining the future of low-mass, core-He-burning hot subdwarfs - JJ Hermes, Boston University
09:20-09:40 (20min)
› Helium Stars, Heavy Metals, High Velocities and Explosions - Simon Jeffery, Trinity College Dublin, Armagh Observatory and Planetarium
09:40-10:00 (20min)
› Helium star donors to thermonuclear supernovae - Josiah Schwab, University of California, Santa Cruz
10:00-10:05 (05min)
› Effect of L3 mass loss on formation of sdB-MS binaries - Alexey Bobrick, Lund Observatory
10:05-10:25 (20min)
Session 3.2: Origin and evolution, progenies and progenitors
Chair: Ingrid Pelisoli
› Formation of hot subdwarf B stars with neutron star components - You Wu, Yunnan Observatories, Chinese Academy of Sciences
10:50-11:10 (20min)
› The Formation and Evolution of R Coronae Borealis Stars - Josiah Schwab, University of California, Santa Cruz
11:10-11:30 (20min)
› Thermal Timescale Mass Transfer and the Growth of Helium White Dwarfs - Evan Bauer, Physics Department, UC Santa Barbara
11:30-11:50 (20min)
› He-shell burning hot subdwarf B stars as candidates for blue large-amplitude pulsations - Xuefei CHEN, Yunnan Observatories
11:50-12:10 (20min)
› BLAPS: the Possible Surviving Companions of Type Ia Supernovae - Xiangcun MENG, Yunnan Observatories, Chinese Academy of Sciences
12:10-12:30 (20min)
