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The Physics of Star Cluster Formation and Evolution
(Springer, 2020)
Gamma-ray emission from star-forming regions
(Società Astronomica Italiana, 2010-04)
Star-forming regions have been tentatively associated with gamma-ray sources since the early days of the COS B satellite. After the many sources detected by the Compton Gamma-Ray Observatory, the statistical evidence for ...
Resolved star formation in the metal-poor star-forming region Magellanic Bridge C
(Oxford University Press, 2020)
Magellanic Bridge C (MB-C) is a metal-poor (similar to 1/5 Z(circle dot)) low-density star-forming region located 59 kpc away in the Magellanic Bridge, offering a resolved view of the star formation process in conditions ...
The lithium-rotation connection in the newly discovered young stellar stream Psc-Eri (Meingast 1)
(European Southern Observatory, 2020)
Context. As a fragile element, lithium is a sensitive probe of physical processes occurring in stellar interiors.
Aims. We aim to investigate the relationship between lithium abundance and rotation rate in low-mass members ...
Quiescent and active phases in Be stars: a WISE snapshot of Young Galactic Open Clusters
(IOP Publishing, 2018-01)
Through the modeling of near-infrared photometry of star-plus disk systems with the codes bedisk/beray, we successfully describe the Wide-Field Infrared Survey Explorer (WISE) photometric characteristics of Be stars in ...