'Chandra harvard edu photo' presentation slideshows

Galaxy Clusters and Large Scale Structure

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M82

M82 . A Study of the galaxies starburst nature and composition. Credit: NASA , ESA and the Hubble Heritage Team STScI / AURA ). Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain ( STScI ) and P. Puxley (NSF). Basic Information.

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Stellar Magnitudes and Distances

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Gravitational lensing of gravitational waves

Gravitational lensing of gravitational waves . In collaboration with M. Hattori & T. Futamase (Tohoku Univ.). . Yousuke Itoh ( RESCEU, U. of Tokyo) seminar@ICRR , 2012 June 26. Affiliation ? Tohoku U.(Prof. Futamase ) ? AEI, Potsdam ? UWM ? Tohoku U. ? RESCEU

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Welcome!

Welcome!. Sun and Seasons. Photo from http://sohowww.nascom.nasa.gov/bestofsoho/bestofsoho.html. Created by the Lunar and Planetary Institute For Educational Use Only LPI is not responsible for the ways in which this powerpoint may be used or altered. What are we going to cover.

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Mass and the Properties of Main Sequence Stars

Mass and the Properties of Main Sequence Stars. M ass is the most important properties of the main-sequence stars. It determine their luminosity, surface temperature, radius, and lifetime.

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Determining the neutrino hierarchy from a galactic supernova using a next-generation detector

Determining the neutrino hierarchy from a galactic supernova using a next-generation detector. http://www.spitzer.caltech.edu/search/image_set/20?search=sig08-016. http://chandra.harvard.edu/photo/printgallery/2004/. http://www.spitzer.caltech.edu/search/image_set/20?search=ssc2005-14c.

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Determining the Neutrino Hierarchy From a Galactic Supernova

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A Search for a Correlation Between Mass Segregation and Metallicity

A Search for a Correlation Between Mass Segregation and Metallicity. Nick DiPreta. Goals. To measure properties of star clusters To learn more about celestial analytic techniques To look for a correlation between metalicity and mass segregation in star clusters.

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http://chandra.harvard.edu/photo/2007/m51/

http://chandra.harvard.edu/photo/2007/m51/. Confronting Stellar Feedback Simulations with Observations of Hot Gas in Elliptical Galaxies . 3-D stellar feedback simulation. NGC 4697: X-ray intensity contours. Q. Daniel Wang, Shikui Tang, Yu Lu, Houjun Mo (UMass)

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By: Amber Shelton

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Life Cycle of a Star

Life Cycle of a Star. Star Life Cycle: Stars are like humans. They are born, live and then die. _____________ _____________ is the total mass of the gas and dust between the stars. Interstellar Medium. NEBULA. _____________: A dense cloud of gas and dust.

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Quark Stars

Quark Stars. Kyle Dolan Astronomy 4001 10 December 2007. NASA/Dane Berry. Outline. Introduction to Quark Stars (QS) Significance of QS Characteristics of QS Possible examples of QS Controversy over the existence of QS Possible future observations. Overview of Neutron Stars.

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Life Cycle of the Stars

Life Cycle of the Stars. By Aiyana and Meredith. http://techcenter.davidson.k12.nc.us/spring026/images/OuterSpace.jpg. Nebula. A nebula is made of gas and dust T he nebula is the birth place of a star They g et their light from nearby stars.

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