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Resolved Stars' Insights into Galaxy Physics
The history of a galaxy is encoded in its individual stars, and resolved stellar populations in nearby galaxies provide a wealth of information about star formation history (SFH), its relation to the interstellar medium, and galactic dynamics/structures. Using the power of resolved stars, imaged in multiple wavelengths by the ...
X-ray Insights into Massive Star Evolution: the X-ray Source Population of M33 as seen by XMM-Newton, Chandra, and the Hubble Space Telescope
Massive stars are key drivers in the cycle of star formation and overall galactic chemical evolution, but many aspects of the evolution of high-mass stars, in particular the end stages of their lifetimes, are difficult to constrain observationally. High-mass X-ray binaries (HMXBs) and supernova remnants (SNRs) are observable ...