Primordial Star Formation

Add to your list(s) Download to your calendar using vCal

• Professor Ralf Klessen, Heidelberg University
• Thursday 30 March 2023, 16:00-17:00
• Hoyle Lecture Theatre, Institute of Astronomy, Madingley Rise.

If you have a question about this talk, please contact Please see programme below.

The first generation of stars, often called Population III (or Pop III ), form from metal-free primordial gas at redshifts z _{30 and below. They dominate the cosmic star formation history until z} 20-15, at which point the formation of metal-enriched Pop II stars takes over. I review current theoretical models for the formation, properties and impact of Pop III stars, and discuss observational constraints. I argue that primordial gas is highly susceptible to fragmentation and Pop III stars form as members of small clusters with a logarithmically flat mass function. Feedback from massive Pop III stars plays a central role in regulating subsequent star formation, but major uncertainties remain regarding its immediate impact. Direct observations of Pop III stars in the early Universe remain extremely challenging, whereas stellar archeological surveys allow us to constrain both the low-mass and the high-mass ends of the Pop III mass distribution. Observations suggest that most massive Pop III stars end their lives as core-collapse supernovae rather than as pair-instability supernovae.

This talk is part of the Kavli Institute for Cosmology Seminars series.

This talk is included in these lists:

• Combined External Astrophysics Talks DAMTP
• Cosmology, Astrophysics and General Relativity
• Hoyle Lecture Theatre, Institute of Astronomy, Madingley Rise
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists

Note that ex-directory lists are not shown.