TY  - GEN 
AU  - Sartorio, Nina S.
AU  - Fialkov, Anastasia
AU  - Hartwig, Tilman
AU  - Mirouh, Giovanni Marcello
AU  - Izzard, Robert G.
AU  - Magg, Mattis
AU  - Klessen, Ralf S.
AU  - Glover, Simon C. O.
AU  - Chen, Li-Hsin
AU  - Tarumi, Yuta
AU  - Hendriks, David D.
PY  - 2023
UR  - https://hdl.handle.net/10481/111726
AB  - The first population of X-ray binaries (XRBs) is expected to affect the thermal and ionization states of the gas in the early Universe. Although these X-ray sources are predicted to have important implications for high-redshift observable signals,...
LA  - eng
PB  - Oxford University Press
KW  - stars: Population III
KW  - (cosmology:) diffuse radiation
KW  - X-rays: binaries
KW  - (cosmology:) early Universe
KW  - Astrophysics - High Energy Astrophysical Phenomena
KW  - Astrophysics - Cosmology and Nongalactic Astrophysics
TI  - Population III X-ray binaries and their impact on the early universe
DO  - 10.1093/mnras/stad697
ER  -