Recent Talks
List of all the talks in the archive, sorted by date.

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BCAM
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It is often assumed that when stars reach their Eddington limit, strong outflows are initiated, and that this happens only for extreme stellar
masses. I will show that in realistic models of stars up to 500 Msun, the Eddington limit is not reached at the stellar surface. Instead, I will argue that the Eddington limit is exceeded inside the stellar envelope, in hydrogen-rich stars above about 1 ... 30 Msun, and in Wolf-Rayet stars above 7 Msun, with drastic effects for their structure and stability. I will discuss the observational evidence for this, and outline evolutionary consequences.

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The epoch of reionization has been predicted to leave an imprint on the star formation histories of dwarf galaxies. I will briefly review theoretical ideas and observational constraints on reionization. I will then discuss the predicted effects on the evolution of dwarf galaxies.
This will be followed by a discussion of tests using star formation histories of nearby dwarf galaxies.
Upcoming talks
- Harmoni IFS Pre-Optics SCT Prototype testsRafael Melgar HernándezFriday April 4, 2025 - 11:30 GMT+1 (Aula)
- Latest Neutrino Achievements and Possible Synergies to Science in the IACProf. Anatael CabreraTuesday April 8, 2025 - 12:30 GMT+1 (Aula)