'4 solar masses' diaporamas de présentation

Phys 1830: Lecture 31

Phys 1830: Lecture 31. Shapely 1, Malin. SNR G21.5-0.9 Bietenholz, Mathewson, Safi-Harb. Office Hour Today 3pm Allen 514. Extra Image-making workshop! April 8, 5:30pm, Allen 536(?). Previous Classes: Stellar Evolution of a 1 solar mass star Radii, Mass, Lifetime on Main Sequence

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Gregory Mendell LIGO Hanford Observatory

Gravitational Waves From Neutron & Strange Quark Stars. Gregory Mendell LIGO Hanford Observatory. Supported by the National Science Foundation. http://www.ligo.caltech.edu. The Neutron Star Idea. SN 1987A.

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Nova & SuperNova

Nova & SuperNova. Heart of the Valley Astronomers, Corvallis, OR 2007. Types of Nova. Type 1a The most commonly accepted theory of this type of supernovae is that they are the result of a carbon-oxygen white dwarf accreting matter from a nearby companion star, typically a red giant.

892 views • 25 slides

Gregory Mendell LIGO Hanford Observatory

Gravitational Waves From Neutron & Strange-quark Stars. A billion tons per teaspoon: the history of neutron stars. The discovery of pulsars and identification with NS. Are NS really strange-quark stars? GWs from NS and SQS. What will we learn?. Gregory Mendell LIGO Hanford Observatory.

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Stellar

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