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SUMMARY:Tracing Star Formation Histories in the Local Neighborhood using Y
 oung Stellar Associations
DTSTART;VALUE=DATE-TIME:20261028T182100Z
DTEND;VALUE=DATE-TIME:20261028T182200Z
DTSTAMP;VALUE=DATE-TIME:20261026T232713Z
UID:indico-contribution-3707@nyx.physics.mcgill.ca
DESCRIPTION:Speakers: Sargun Jassal (University of Toronto)\nYoung stellar
  associations provide an opportunity to investigate the recent star format
 ion history of the Solar Neighborhood by identifying groups of stars that 
 share similar ages and kinematic properties. In this work\, I investigate 
 two nearby young stellar associations\, SCYA 75 (Ophiuchus Southeast) and 
 SCYA 103 (Scorpius-Centaurus)\, to explore whether their stellar populatio
 ns show evidence of differences in their formation histories. I used a loc
 al k-neighborhood search to identify nearby stellar members and characteri
 ze the local stellar populations associated with each region. I then compa
 red the age distributions and statistical properties of the identified pop
 ulations to investigate similarities and differences between the two assoc
 iations. By examining the ages of stars in these neighboring regions\, thi
 s study aims to provide insight into the timing and structure of recent st
 ar formation in the local solar environment. This approach demonstrates ho
 w spatially localized stellar population searches can be used to connect i
 ndividual young associations to the broader star formation history of the 
 Solar Neighborhood.\n\nhttps://nyx.physics.mcgill.ca/event/587/contributio
 ns/3707/
LOCATION:Online 
URL:https://nyx.physics.mcgill.ca/event/587/contributions/3707/
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