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In this episode Dr Ezzeddine told me about how the chemical and physical compositions of stars can be inferred by the use of spectroscopy. Additionally, she explained what the r-process is, and how by building radiative transfer models we can calculate the abundances of elements in the atmospheres of stars.
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حلقات أخرى في هذا البودكاست
This episode Dr Du spoke about some of her work looking at the physical properties of the interstellar medium in distant galaxies. She also spoke about her interest in asgtronomy outreach and the kind of work she does as outreach manager at the Kavli Institute for Particle Astrophysics and Cosmolog…
Active galactic nuclei are found in the centers of galaxies and emit extremely high levels of radiation, which Dr Hervet tries to model computationally. Dr Hervet is also part of the VERITAS collaboration which is a ground based observatory with an array of 4 telescopes, each with a 12 meter wide d…
In this episode Dr Estrela spoke about her research into classifying and charecterizing the atmospheres of exoplanets, and also her research the effects of stellar activity on these exoplanets. Dr Estrela explained how she first was interested in astrobiology and how her work is helping us answer t…
Dr Daylan, told me about his work on explanets utilising primarily the TESS mission, and how the transit method is used to discover these planets. Additionally, he also spoke about the charecteristics that can be inferred from a discovered planets, such as the mass, density and orbital radius.
إخلاء المسؤولية: البودكاست والأعمال الفنية المضمنة في هذه الصفحة مأخوذة من Vikram Bhamre، وهي مملوكة لمالكها وليست تابعة لشركة Listen Notes, Inc أو معتمدة منها.
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