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Sivan Ginzburg
Hebrew University of Jerusalem
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Illustration of a star orbiting a white dwarf
Stellar Evolution
Stars evolve through a variety of stages. For example, our sun's envelope will inflate by orders of magnitude to become a red giant, leaving behind a dense white dwarf core the size of the Earth. We study the evolution of various stars, focusing on binary systems where two different stars closely orbit one another and interact.
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Directly-imaged planet inside its birth disk
Exo-planets
The first planet orbiting another sun was discovered in 1995, and thousands more were detected since. In 2018, astronomers have directly imaged a planet during its formation for the first time. We use stellar evolution tools to study planet formation and evolution, focusing on directly-imaged planets.
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