BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Heidelberg University//HePhySTO//EN
CALSCALE:GREGORIAN
BEGIN:VEVENT
DTEND:20260709T101500Z
UID:746d13c027ed376ddaaf6ffc62d9b74b@physik.uni-heidelberg.de
DTSTAMP:20260411T171036Z
LOCATION:ARI\, Moenchhofstrasse 12-14\, Seminarraum 1.OG
DESCRIPTION:I will review the recent progress that we have made in understa
 nding nucleosynthesis in the Universe and the accretion history of the Milk
 y Way through chemodynamical analysis of the stellar halo. Over the last fi
 ve years\, we have been complementing the discoveries from the Gaia mission
  with high-resolution spectroscopic follow-ups of halo stars. These studies
  have provided detailed chemical abundances of stars in stellar streams\, r
 evealing the origins of these streams. There have also been serendipitous d
 iscoveries during these follow-ups leading to new insights into broader top
 ics in astrophysics\, such as the discovery of Li-rich stars in stellar str
 eams and the association of a 33 Msun solar mass black hole with a stellar 
 stream. After reviewing these discoveries\, I will discuss the future prosp
 ects of this field in light of the recently started spectroscopic surveys\,
  namely 4MOST and WEAVE\, hopefully with initial results from them by the t
 ime of the colloquium. Finally\, I will briefly introduce the next generati
 on spectroscopic facilities that are currently being discussed. In addition
  to these scientific topics\, I will also share my personal experience of b
 eing a Gliese fellow at ARI for three years and how it has impacted my care
 er.\n\nImported from https://www.physik.uni-heidelberg.de/hephysto/ (no war
 ranty for accuracy).
URL;VALUE=URI:https://www.physik.uni-heidelberg.de/hephysto/index.php?s=tal
 k&id=12574
SUMMARY:ARI Institute Colloquium: Tadafumi Matsuno - Nucleosynthesis and th
 e Milky Way&apos\;s accretion history: What we have learned and what we wil
 l learn
DTSTART:20260709T091500Z
END:VEVENT
END:VCALENDAR