TY  - GEN 
AU  - Goswami, Sabyasachi
AU  - Vilchez, J.M.
AU  - Pérez-Díaz, B.
AU  - Silva, L.
AU  - Bressan, A.
AU  - Pérez-Montero, E.
A4  - Física Aplicada
PY  - 2024
SN  - 1432-0746
SN  - 0004-6361
UR  - http://hdl.handle.net/10498/35543
AB  - Context. Recent work presented increasing evidence of high non-constant S/O abundance ratios observed in star-forming metal-poor galaxies that deviated from the constant canonical S/O across a wide range of O/H abundances. Similar peculiarly high Fe/O...
LA  - eng
PB  - EDP Sciences
KW  - Galaxies: luminosity function, mass function
KW  - Galaxies: starburst;
KW  - Galaxy: abundances;
KW  - Stars: massive;
KW  - Stars: Population II;
KW  - Stars: Population III
TI  - Contribution of very massive stars to the sulfur abundance in star-forming galaxies: Role of pair-instability supernovae
DO  - 10.1051/0004-6361/202348231
ER  -