'Small magellanic cloud' presentation slideshows

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An analysis of the H I component of the Magellanic Bridge

An analysis of the H I component of the Magellanic Bridge. Erik Muller: University of Wollongong Australia Telescope National Facility Supervisors: Bill Zealey (UOW) Lister Staveley-Smith (ATNF). Overview: H I observations of the Magellanic Bridge.

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Galaxies

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Bars Galaxy and galactic system mergers Stefans Quintet impulse approximation

AST1420. Lecture 19 Bars, Mergers, Ellipticals. Bars Galaxy and galactic system mergers Stefans Quintet impulse approximation dynamical friction dynamical friction in Maxwellian velocity field applications: dissolution of globular clusters in Andromeda

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Hubble Science Briefing

Hubble Science Briefing. 30 Doradus: Birthplace of giants and dwarfs. Elena Sabbi. June 7, 2012. Outline. How stars form and evolve; How we can use star clusters to better understand high redshift galaxies; Characteristics of the Large Magellanic Cloud;

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Part 5: The Galaxy and the Universe

Part 5: The Galaxy and the Universe. In this final part of the course, we will: 1. Look at the big spatial picture : Are there organizations of stars? What is the size of the universe? If it is finite, is there an edge? 2. Look at the big temporal picture :

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Th e Universe: Galaxies

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Spiral Galaxies

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ASTRONOMY 310

ASTRONOMY 310. TAs Frank Berghaus fbergh@physics.ubc.ca Marie-Andree Dumais madumais@physics.ubc.ca Jillian Henderson jhenders@physics.ubc.ca Simon Kras skras@physics.ubc.ca. Lectures and Tutorials Lectures: MWF 12:00 Hebb Theatre Tutorials: as registered. Alternate weeks beginning Jan 19

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WHERE HAVE ALL THE GIRLS GONE? Nina Byers

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El universo :

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1B11 Foundations of Astronomy Cosmic distance scale

1B11 Foundations of Astronomy Cosmic distance scale. Liz Puchnarewicz emp@mssl.ucl.ac.uk www.ucl.ac.uk/webct www.mssl.ucl.ac.uk/. 1B11 Cosmic distance scale. Why is it so important to establish a cosmic distance scale?

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Where Are We?

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Stellar Motion

Stellar Motion. Stellar Motion. Apparent Motion The apparent motion of stars is the motion visible to the unaided eye. Apparent motion is caused by the movement of Earth.

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The Topology of HI in the SMC

The Topology of HI in the SMC. Jeremy Gordon University of Georgia August 2, 2007 Advisors: Dr. Chepurnov Dr. Lazarian. Overview:. Small Magellanic Cloud Genus Statistics HI Column Density Map My Project Results. The Small Magellanic Cloud. NGC 292

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Lecture 2 Astronomy Today

Lecture 2 Astronomy Today. 1 nanosecond = 1 ft. (1/1,000,000,000 second ). Light Speed = 299,792,458 meters/second. Using Light to Measure Distance. Earth to Moon = 1.28 light seconds. Light Speed = 299,792,458 meters/second. Using Light to Measure Distance.

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Life Cycles of Stars

Life Cycles of Stars. The Hertzsprung-Russell Diagram. How Stars Form. Collapsing gas and dust cloud Protostar - mostly infrared. Main Sequence Stars. Brown Dwarf Red Dwarf Normal Star. All Objects Exist Because of a Balance Between Gravity and Some Other Force.

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Tour of the Universe!

Tour of the Universe!. Andromeda:.

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Planetary Nebulae as tracers of SMC formation

1. THE DATA. 2. DETERMINATION OF AGE-ABUNDANCE RELATIONS. Planetary nebulae sample observed between 1999 and 2002. 1) Effective temperature ( T eff ). 2) Luminosity ( L/L ? ). of each PN central star. Object. Date. Site. E(B-V). Age derivation for PNe.

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