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Richard Pogge - Jan 31: Extreme Stars: White Dwarfs & Neutron Stars mp3

Richard Pogge - Jan 31: Extreme Stars: White Dwarfs & Neutron Stars mp3

MP3 2888 mb. | FLAC 2810 mb. | WMA 1839 mb.

Interprète: Richard Pogge
Titre: Jan 31: Extreme Stars: White Dwarfs & Neutron Stars
Publié sur: 2006
Style: Spoken Word, Education
Catégorie: Non musique
Classement: 4.7
Label: Not On Label (Richard Pogge Self-released)

Tracklist

1Jan 31: Extreme Stars: White Dwarfs & Neutron Stars42:15


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

This lecture introduces these stellar remnants: White Dwarfs remnants of low-mass stars held up by Electron Degeneracy Pressure, and Neutron Stars remnant cores of core-bounce supernovae held up by Neutron Degeneracy Pressure. We also the Chandrasekhar Mass for White Dwarfs, Type Ia Supernovae resulting from a white dwarf getting tipped over the Chandrasekhar Mass, Pulsars rapidly rotating magnetized neutrons stars, and ask what happens when a neutron star gets tipped over its mass limit. Recorded 2006 January 31 in 1008 Evans Laboratory on the Columbus campus of The Ohio State Universit. Слушайте Astronomy 162 - Stars, Galaxies, & the Universe в подкасте Richard Pogge на любом устройстве с приложением myTuner video is about the differences between the corpses or final degenerate dense star forms that dead stars take: black holes, neutron stars, and white dwarfs. The main distinguishing features between them are the mass cutoffs Chandrasekhar limit and Tolman-Oppenheimer-Volkoff Limit. Neutron Stars - The Neutron Stars. Лента с персональными рекомендациями и музыкальными новинками, радио, подборки на любой вкус, удобное управление своей коллекцией. 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. Related Music albums to Jan 31: Extreme Stars: White Dwarfs & Neutron Stars by Richard Pogge. Richard Pogge - Lecture 2: Astronomical Numbers 2. Richard Pogge - Lecture 23: Worlds Within: Atoms 2007 Oct 23 3. Richard Pogge - Jan 23: Energy Generation & Transport In Stars 4. Turner - Billions And Billions Of Stars And Galaxies. Richard Strauss - Till Eul. Timeline of neutron stars, pulsars, supernovae, and white dwarfs. Note that this list is mainly about the development of knowledge, but also about some supernovae taking place. For a separate list of the latter, see the article List of supernovae. All dates refer to when the supernova was observed on Earth or would have been observed on Earth had powerful enough telescopes existed at the time. 185 Chinese astronomers become the first to record observations of a supernova, SN 185. TracksFree Non Music Richard Pogge - Jan 31: Extreme Stars: White Dwarfs & Neutron Stars. Singer: Richard Pogge Album title: Jan 31: Extreme Stars: White Dwarfs & Neutron Stars Label: Not On Label Richard Pogge Self-Date of released none Series: Astronomy 162: Introduction To Stars, Galaxies, & The Universe - Lecture Audio Podcasts - Winter 2006 , Unit 3: Death & Transfiguration Type: File, MP3, Mono, VBR Country: Date of released: 2006 Category: Non-Music Style: Spoken Word, Education Rating . If others are interested in listening to them, please point them to this URL. Jan 31: Extreme Stars: White Dwarfs & Neutron Stars. Feb 1: Black Holes. Feb 2: Testing Stellar Evolution. The Neutron Stars, New York, New York. New York based music duo of Thomas Hutchings & Richard Wendel heavily influenced by Massive Attack. This video is from my album The Neutron Stars HYBRID Written by Richard Lee Wendel and Tanya Michelle Produced by Richard Lee Wendel and Thomas Hutchings F. Mailing out pre-order Hybrid CDs & Tshirts . Neither neutron stars nor black holes, despite their mass, can be considered stars. ESOLuís Calçada. When it comes to stars, there's a huge variety of different types out there. Our Sun is nothing spectacular, as there are stars both redder and bluer, brighter and dimmer, and more-or-less massive by great amounts. White dwarf stars - and their far-future versions known as black dwarfs - are stellar remnants, rather than true stars themselves. Even when matter accretes on the surface of a white dwarf and flares up with fusion, creating a nova, it cannot be considered a star. Stars have fusion occur in their core surface fusion simply will not do