'Blue stars' presentation slideshows

Properties of Stars

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Lecture 5 Outline

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Making a Color-Magnitude Diagram for Globular Cluster Omega Centauri

Making a Color-Magnitude Diagram for Globular Cluster Omega Centauri. Jay Anderson, STScI. 1. This is the Early-Release Image of Omega Centauri, taken by WFC3/UVIS on board the Hubble Space Telescope (HST). http://hubblesite.org/gallery/wallpaper/pr2009025q/. 2.

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Making a Color-Magnitude Diagram for Globular Cluster Omega Centauri

Making a Color-Magnitude Diagram for Globular Cluster Omega Centauri. Jay Anderson, STScI. 1. This is the Early-Release Image of Omega Centauri, taken by WFC3/UVIS on board the Hubble Space Telescope (HST). http://hubblesite.org/gallery/wallpaper/pr2009025q/. 2.

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Bellwork

Bellwork. 1. Define AU 2. What do we call the 3 Laws of Planetary Motion?. Chapter 3 Section 4 Planetary Motion Review. Visual Concepts online Ch3Sec4 Planetary Motion worksheet. Create a Chart.

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An overview of the AEOS Burst Camera

An overview of the AEOS Burst Camera. Heather Swan University of Michigan June 3, 2005. 1. Outline. Science Goals System design GRB Triggers/Response Grating analysis/Simulations. 2. AEOS Burst Camera Sensitivity. ROTSE-I/TAROT. Half of all GRBs have no optical counterparts

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Characteristics of stars

Characteristics of stars. 4.? The structure and composition of the universe can be learned from studying stars and galaxies and their evolution. As a basis for understanding this concept: a. Students know galaxies are clusters of billions of stars and may have different shapes.

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X-ray gas

UV. X-ray gas. Molecular gas. Cool gas. Optical filaments. Star formation. Blue continuum. Carolin Crawford ? IoA, Cambridge. Central cluster galaxies. Optical emission-line gas. Crawford et al 1999. RXJ1532.9. Z3146. A2204. A1835. Conselice et al 2001.

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Chapter 30 Section 1 Stars, Galaxies and the Universe

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Philamentary Structure and Velocity Gradients in the Orion A Cloud

Red: CO from Mini survey. Philamentary Structure and Velocity Gradients in the Orion A Cloud. Spitzer Orion Cloud Survey: 10 sq. degrees in Orion A and Orion B mapped between 2004-2009 IR-ex: 3352 IR-ex + coup: 3845 IR-ex + coup + corr: 4300 Megeath et al. (y+1) y = current year. Orion B.

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3 Models for Subtraction Algorithms

3 Models for Subtraction Algorithms. By Kim Iverson. Subtraction. Subtraction is usually explained as the taking away of a subset of objects from a given set. . Subtraction.

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Light: Thermal Spectra Emission and Absorption Spectra

Light: Thermal Spectra Emission and Absorption Spectra. Recap. Canvas homework due FRIDAY Lab this week: the Hertzsprung -Russell diagram (unfortunately, getting here a little ahead of class!)

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M-31 The Andromeda Galaxy

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This is what you see when you look up at the night sky!

S. T. A. R. S. This is what you see when you look up at the night sky!. Millions of stars! Too many to count!. Look closer at the stars!. Look even closer at this star!. CLOSER!!!. A star is simply a ball of hot burning gases. There are 3 colors of stars. red. yellow. blue.

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Planets Inner vs. outer

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Kindergarten Orientation

Kindergarten Orientation. 2013-2014. Welcome to Kindergarten!. Pencil instead of homework pass Paperwork from office & PTG membership send back ASAP Who has permission to pick up your child send back ASAP Class List Extra Information. Attendance.

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Giorgio Bianciardi University of Siena

Life in the Universe #2_2. Giorgio Bianciardi University of Siena. Life beyond the Earth: the solar system. 1976 Viking #1 Viking #2. Life on Mars ?. ALH84001. Life on Mars (billion years ago)?! D.S. Mc Kay, Science, 1996. PAH. Beyond Mars. Titan: a Saturn moon. Jupiter moons.

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SPACE AND BEYOND

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The Night Sky

The Night Sky. By: Nathan, Bailey, Alyvia and Brianna. Constellations. There are stars in the sky. Stars that form shapes are called constellations. There are many constellations in the sky. This one is called Orion. He is a warrior. Stars.

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