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Richard Pogge - Feb 14: Groups & Clusters Of Galaxies mp3

Richard Pogge - Feb 14: Groups & Clusters Of Galaxies mp3

MP3 1306 mb. | FLAC 1899 mb. | WMA 2460 mb.

Interprète: Richard Pogge
Titre: Feb 14: Groups & Clusters Of Galaxies
Publié sur: 2006
Style: Spoken Word, Education
Catégorie: Non musique
Classement: 4.8
Label: Not On Label (Richard Pogge Self-released)

Tracklist

1Feb 14: Groups & Clusters Of Galaxies39:22


Notes

These lecture podcasts are audio recordings of daily lectures from Prof. Richard Pogge's Winter Quarter 2006 section of Astronomy 162 at The Ohio State University. They were recorded live, unscripted and unedited.


Album

Galaxy groups and clusters are the largest known gravitationally bound objects to have arisen thus far in the process of cosmic structure formation. They form the densest part of the large-scale structure of the Universe. In models for the gravitational formation of structure with cold dark matter, the smallest structures collapse first and eventually build the largest structures, clusters of galaxies. Groups and. Galaxies are found in groups and clusters, and these are only the start of a hierarchy of cosmic structures up to the largest scales observed. This lecture introduces the properties of groups and clusters of galaxies, superclusters clusters of clusters, and large scale structure with filaments of superclusters surrouning vast voids. We start with our Local Group, and then expand our view to encompass the depths of intergalactic space. Recorded 2006 February 14 in 1008 Evans Laboratory on the Columbus campus of The Ohio State University. Two colliding groups of galaxies located about 380 million light years from Earth. 26 Nov 19. Positive Feedback Black Hole. A galaxy located about 9. 9 billion light years from Earth. 18 Nov 19. Phoenix Cluster. A galaxy cluster located about 5. 8 billion light years from Earth. A giant collection of galaxies immersed in hot gas about 250 million light years from Earth. 03 Apr 14. El Gordo. A galaxy cluster nicknamed El Gordo about 7 billion light years from Earth. 04 Mar 14. ESO 137-001. Galaxy ESO 137-001 plunges through the Norma galaxy cluster. Слушайте Astronomy 162 - Stars, Galaxies, & the Universe в подкасте Richard Pogge на любом устройстве с приложением myTuner to music from Richard Pogge like Lecture 38: The First Three Minutes. Find the latest tracks, albums, and images from Richard : Richard Pogge Title: Feb 14: Groups & Clusters Of Galaxies Released: 2006 Style: Spoken Word, Education Rating: 4. 2 Votes: 878 Other formats: ADX MIDI AUD MPC AC3 TTA DMF. Richard Pogge Spoken Word Education 2006. Download links. Richard Pogge - Feb 14: Groups & Clusters Of Galaxies MP3 album ZIP archive. Richard Pogge - Feb 14: Groups & Clusters Of Galaxies FLAC album ZIP archive. Richard Pogge - Feb 14: Groups & Clusters Of Galaxies WMA album ZIP archive. Feb 14: Groups. This is part of my complete intro Astronomy class. If you want to watch all the videos in the correct order, please visit my website by marking Clusters and Groups of Galaxies as Want to Read: Want to Read saving Want to Read. Currently Reading. Clusters and Groups of. by F Mardirossian. Wed love your help. Let us know whats wrong with this preview of Clusters and Groups of Galaxies by F Mardirossian. Galaxies like company - Galaxies invariably form groups, and groups form clusters, and clusters form superclusters. Gravity is at the core of this tendency. When a large galaxy forms, its massive gravitational field captures smaller galaxies that have formed in its vicinity. Then our local group, which includes Andromeda our group is fairly unusual in having two large galaxies, has a gravitational connection with several other groups that together form the Virgo Cluster, so-called because they all appear in the constellation Virgo. Astrophysics of Galaxies. Authors and titles for recent submissions. Tue, 30 Jun 2020. Subjects: Astrophysics of Galaxies Earth and Planetary Astrophysics High Energy Astrophysical Phenomena Solar and Stellar Astrophysics . arXiv:. Title: GASP XXI. Star formation rates in the tails of galaxies undergoing ram-pressure stripping