2025-05-28

Speaker: Soetkin Janssens (RESCEU, U. Tokyo)

Abstract:

Massive stars play an important role in the evolution of galaxies. With masses larger than eight times the mass of the Sun, these stars regulate galaxy-wide feedback and star formation. They end their lives with a violent supernova, leaving behind a compact object — neutron star of black hole. The formation of black holes is however insufficiently understood, largely due to a limited number observations. While over ten million black holes are predicted to reside in the Milky Way, only very few have been discovered so far. Moreover, in the past years, several black-hole imposters were discovered, highlighting the difficulty of the black-hole search. However, this search is far from over and the coming years may be very promising. While our current methods are very slowly becoming fruitful, a new method is on the way that may uncover hundreds of black holes at once based on astrometric data from the Gaia space telescope. This will reveal how black holes form and will help us to better understand the evolution towards gravitational wave mergers. 

2025-05-21

Speaker: Yuki Isobe (Cambridge University)

Abstract:

Chemical abundance ratios in the interstellar medium of galaxies trace the accumulated contributions of stars with varying masses, serving as key indicators of early star formation. In particular, nitrogen-to-oxygen (N/O) and iron-to-oxygen (Fe/O) ratios have generally been thought to increase with galaxy age: massive stars initially eject oxygen via core-collapse supernovae, while later contributions from lower-mass stars enhance nitrogen and iron abundances. However, this standard evolutionary scenario has been challenged by recent spectroscopic observations using the James Webb Space Telescope (JWST) and large ground-based telescopes. This talk will review these findings across cosmic time, particularly z~0 extremely metal-poor emission-line galaxies with ~solar Fe/O ratios and z>5 galaxies with supersolar N/O ratios. I will also discuss a connection between nitrogen enhancement, dense gas, and active galactic nuclei, providing new insights into early chemical enrichment, clustered star formation, and massive black hole seeding in the early Universe.