As a brief revision, the origin of heavy elements and the role of abundances in extremely metal-poor (EMP) stars are presented. Heavy element abundances in the EMP uranium-rich star CS 31082-001 based mainly on near-UV spectra from STIS/HST are presented. These results should be useful for a better characterisation of the neutron exposure(s)...
-
May 19, 2013 (v1)Conference paperUploaded on: December 4, 2022
-
September 10, 2019 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
August 20, 2019 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
October 24, 2023 (v1)Journal article
Context. Classical Cepheids (CCs) are solid distance indicators and tracers of young stellar populations. Dating back to the beginning of the 20th century, they have been safely adopted to trace the rotation, kinematics, and chemical enrichment history of the Galactic thin disk. Aims. The main aim of this investigation is to provide iron,...
Uploaded on: April 4, 2025 -
January 10, 2019 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
October 1, 2021 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
February 9, 2021 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
June 9, 2021 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
June 1, 2020 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
December 20, 2016 (v1)Journal article
International audience
Uploaded on: December 3, 2022