Culips English Podcast: Practical English Learning Made Fun Learn and Explore: Join Culips for an exciting English learning journey. Our podcast focuses on teaching English idioms, slang, and phrasal verbs through fun and engaging conversations. Each episode helps you master English for real-life situations. Unique Learning Experience: Culips stands out by blending language skills with cultural insights. Our diverse hosts make learning relatable, covering a variety of everyday topics. You’ll ...
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Lecture 25: A Tale of Two Galaxies, The Milky Way and Andromeda
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Content provided by Richard Pogge. All podcast content including episodes, graphics, and podcast descriptions are uploaded and provided directly by Richard Pogge or their podcast platform partner. If you believe someone is using your copyrighted work without your permission, you can follow the process outlined here https://ro.player.fm/legal.
Andromeda is the nearest bright spiral galaxy to the Milky Way, and a near twin in terms of stellar and gas content. This lecture discusses the idea of stellar populations and chemical evolution in galaxies as determined by combining observations from within (the Milky Way) and without (Andromeda). At the end, two other features of these galaxies, their supermassive central black holes, is introduced, setting up a question to be addressed in later lectures. Recorded 2006 February 9 in 1008 Evans Laboratory on the Columbus campus of The Ohio State University.
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43 episoade
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Manage episode 1022686 series 8847
Content provided by Richard Pogge. All podcast content including episodes, graphics, and podcast descriptions are uploaded and provided directly by Richard Pogge or their podcast platform partner. If you believe someone is using your copyrighted work without your permission, you can follow the process outlined here https://ro.player.fm/legal.
Andromeda is the nearest bright spiral galaxy to the Milky Way, and a near twin in terms of stellar and gas content. This lecture discusses the idea of stellar populations and chemical evolution in galaxies as determined by combining observations from within (the Milky Way) and without (Andromeda). At the end, two other features of these galaxies, their supermassive central black holes, is introduced, setting up a question to be addressed in later lectures. Recorded 2006 February 9 in 1008 Evans Laboratory on the Columbus campus of The Ohio State University.
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43 episoade
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