In force date
Call year
2015
Investigator
Sara Rodríguez Berlanas
Financial institution
Financing program
Financing subprogram
Amount granted to the IAC Consortium
3.439,00 €
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Physical properties and evolution of Massive Stars
This project aims at the searching, observation and analysis of massive stars in nearby galaxies to provide a solid empirical ground to understand their physical properties as a function of those key parameters that gobern their evolution (i.e. mass, spin, metallicity, mass loss, and binary interaction). Massive stars are central objects to
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