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Disentangling the Formation Pathways of Protostars
(2023-05)
Star formation occurs within dense cores within molecular clouds, often associated with filamentary structures. However, there exist isolated instances of star formation, far from nearby forming stars. As a core collapses, ...
The Initial-Final Mass Relation Revisited: A Monte Carlo Approach with the Addition of the M67 White Dwarf Population
(2018-12)
The initial-final mass relation (IFMR) describes how the initial mass of a stellar
object maps to its mass as a remnant. The focus of this work is to re-examine this
relation for low to intermediate mass stars.
Studies ...