'1 solar mass' diaporamas de présentation

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Phys 1830: Lecture 29

Phys 1830: Lecture 29. Shapely 1, Malin. Previous Classes: Radii, Mass, Lifetime on Main Sequence This class: Stellar evolution: star birth and death of a star with 1 solar mass. Next Classes: Stellar Evolution: more massive stars Supernovae Type ! Supernovae Type II black holes

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Goal: To understand the post main sequence evolutions of the most massive stars

Goal: To understand the post main sequence evolutions of the most massive stars. Objectives: To learn about Eta Carinae and LBVs To learn about what Wolf-Rayet stars are To understand the effects these stars have on their surroundings and why they are important for the evolution of the galaxy

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Constraints on a Universal IMF 1 from the Entire Stellar Population 2,3

Constraints on a Universal IMF 1 from the Entire Stellar Population 2,3. Ivan Baldry. Johns Hopkins University working with Karl Glazebrook. 1 Assuming a universal IMF and constraining the upper-mass IMF slope (M >~ 1 solar mass).

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Some info and problems to go with last nights presentation on Extrasolar planets.

Some info and problems to go with last nights presentation on Extrasolar planets. I worked on this most of the day today. I plan to use some of this in my class presentation . Jim Honeycutt. Properties of Ellipses. semi-major axis = a 2 times a is the length of major axis.

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Alpha centauri

By: Megan Devin. Alpha centauri. Fun Facts About Alpha Centauri. Member of the triple star system closest to our sun 3rd brightest star in the sky Apparent visual magnitude = -0.3 Proxima Centauri is the closest star to the sun. Fun Facts (Contd.).

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