STARS II: current challenges, upcoming solutions

Session

Session: Chemistry of resolved stellar populations

16 Jun 2025, 10:30

Bologna

135. Invited talk

Sara Lucatello (Istituto Nazionale di Astrofisica (INAF))

16/06/2025, 10:30

136. The early chemical evolution of the Sagittarius dwarf galaxy

Dr Federico Sestito (University of Hertfordshire)

16/06/2025, 11:10

137. High-resolution spectroscopy of metal-poor stars in the Small Magellanic Cloud

Lorenzo Santarelli (Dipartimento di Fisica e Astronomia - Università di Bologna (DIFA - UniBo))

16/06/2025, 11:30

138. CERES survey: chemical abundances of light neutron capture elements

Linda Lombardo (Goethe University Frankfurt)

16/06/2025, 11:50

139. The Bulge Cluster Origin (BulCO) survey: first results in Liller 1

Lanfranco Chiappino (Istituto Nazionale di Astrofisica (INAF))

16/06/2025, 12:10

131. Invited talk

Donatella Romano (Istituto Nazionale di Astrofisica (INAF))

16/06/2025, 14:00

132. Europium, do we have a problem? Modelling r-process enrichment across Local Group galaxies

Marco Palla (University of Bologna, INAF-OAS)

16/06/2025, 14:40

133. Unveiling the Chemical Enrichment with CRIMSONS

Martina Rossi (Istituto Nazionale di Astrofisica (INAF))

16/06/2025, 15:00

134. Unravelling the chemical abundance patterns of the Milky Way building blocks

Alice MORI (Dipartimento di Fisica e Astronomia, Università di Firenze)

16/06/2025, 15:20

140. Homogenous chemical characterisation of accreted streams in the local stellar halo

Emma Dodd (Institute for Computational Cosmology, Durham University)

16/06/2025, 16:10

141. Tracing the evolution of the Milky Way through high-resolution spectroscopy

Edoardo Ceccarelli (Istituto Nazionale di Astrofisica (INAF))

16/06/2025, 16:30

142. A Sequoia Candidate with Exceptionally High Be and Li Abundances: Hypernova or Planetary Engulfment?

Lorenzo Monaco (Istituto Nazionale di Astrofisica (INAF))

16/06/2025, 16:50

143. Icarus Revisited: An Ancient, Metal-poor Accreted Stellar Stream in the Disk of the Milky Way

Paola Re Fiorentin (Istituto Nazionale di Astrofisica (INAF))

16/06/2025, 17:10