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Unit 4: The Universe

Unit 4: The Universe

  • tatyana-admore
  • 12 Slides

Essential Question: 6. Essential Question 6:. Whe...

Active Galaxies

Active Galaxies

  • debby-jeon
  • 14 Slides

Most of the power of galaxies come from the stars...

Sombrero Galaxy (M104)

Sombrero Galaxy (M104)

  • calandra-battersby
  • 6 Slides

Cristian Calderon. What is it?. The sombrero gala...

How Light Spreads Out

How Light Spreads Out

  • trish-goza
  • 11 Slides

Lesson 4. What’s the deal?. The Sun is one medi...

1 What else is in the sky?

1 What else is in the sky?

  • stefany-barnette
  • 22 Slides

2. The Universe. Th. 3. The Universe is . everyth...

Galaxy Consulting

Galaxy Consulting

  • myesha-ticknor
  • 37 Slides

Eleonora Babayants, MLS. Information Overload and...

Astrophysics Focused Telescope Assets (AFTA

Astrophysics Focused Telescope Assets (AFTA

  • mitsue-stanley
  • 72 Slides

). Presentation to P. Hertz April 19, 2013. . ...

Face on illustration of the Milky Way galaxy, showing the prominent sp

Face on illustration of the Milky Way galaxy, showing the prominent sp

  • stefany-barnette
  • 100 Slides

Illustration: CXC/M.Weiss The Galaxy's bright stel...

How do galaxy stellar haloes form?

How do galaxy stellar haloes form?

  • danika-pritchard
  • 100 Slides

A comparison between stateoftheart simulations and...

Project Based Learning

Project Based Learning

  • debby-jeon
  • 29 Slides

Galaxy Bazaar. A social entrepreneurship venture....

Galaxies

Galaxies

  • ellena-manuel
  • 12 Slides

Ms. Cordaro . SMHS . Earth Science. Review/Warm u...

Galaxies

Galaxies

  • trish-goza
  • 53 Slides

The Hubble Tuning-Fork Diagram. This is the tradi...

A Critical Role for Viscosity in the Radio Mode AGN Feedbac

A Critical Role for Viscosity in the Radio Mode AGN Feedbac

  • giovanna-bartolotta
  • 9 Slides

Paul Nulsen. Harvard-Smithsonian Center for Astro...

BULGE FRACTION AND DISTRIBUTION OF STAR FORMATION IN SAMI G

BULGE FRACTION AND DISTRIBUTION OF STAR FORMATION IN SAMI G

  • lindy-dunigan
  • 15 Slides

Greg Goldstein. PhD student, . Dept. of Physics ...

Milky Way thin disk

Milky Way thin disk

  • sherrill-nordquist
  • 30 Slides

Q: in order to study the spatial distribution of ...

Density and temperature conspire to have higher ionization

Density and temperature conspire to have higher ionization

  • aaron
  • 1 Slides

below. ); this qualitative behavior is seen for a...

Conclusions from Galaxy Data

Conclusions from Galaxy Data

  • mitsue-stanley
  • 59 Slides

11. . What do you observe about the direction of ...

The Search for Extraterrestrial Intelligence

The Search for Extraterrestrial Intelligence

  • pamella-moone
  • 20 Slides

The Search for Extraterrestrial Intelligence (SET...

Astrology

Astrology

  • tatyana-admore
  • 8 Slides

Extraterrestrials. CELESTIAL BODIES. Astronomy th...

Nearby Galaxy Evolution

Nearby Galaxy Evolution

  • tawny-fly
  • 8 Slides

Prof. Gerhardt R Meurer. Galaxy evolution in a nu...

Python: Programming the Google Search

Python: Programming the Google Search

  • tawny-fly
  • 58 Slides

Damian Gordon. Ref: Donaldson. , 2013, Python: Vi...

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

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

  • debby-jeon
  • 16 Slides

Confronting Stellar Feedback . Simulations with O...

Gas Detection in Galaxies and Techniques

Gas Detection in Galaxies and Techniques

  • lois-ondreau
  • 9 Slides

C. omparisons. Advisors: David . Frayer. and Ron...

Baryon content of galaxy groups

Baryon content of galaxy groups

  • lindy-dunigan
  • 23 Slides

Ming Sun . (University of Virginia). ‏. M. . ...

14-The Evolution of Stars and Gas in Galaxies

14-The Evolution of Stars and Gas in Galaxies

  • jane-oiler
  • 34 Slides

Elliptical Galaxies. Spiral Galaxies. Barred Spir...

The Baryon Cycle on

The Baryon Cycle on

  • trish-goza
  • 20 Slides

FIRE . Tracing . Cosmic Inflows, Galactic Outflow...

Fast radio bursts and the magnetization and turbulence of t

Fast radio bursts and the magnetization and turbulence of t

  • giovanna-bartolotta
  • 19 Slides

w. eb . Ryan Shannon, . ICRAR-Curtin/. ATNF (. Vi...

CMB cluster lensing

CMB cluster lensing

  • pamella-moone
  • 15 Slides

Towards the first detection using SPT polarisatio...

Probing Dark Dwarf Galaxies with Gravitational Lensing

Probing Dark Dwarf Galaxies with Gravitational Lensing

  • calandra-battersby
  • 56 Slides

Kaiki Taro Inoue . (KINDAI U.). Seminar. @Osaka U...

Important Stuff (Section

Important Stuff (Section

  • liane-varnes
  • 69 Slides

001). The Final Exam is. . Thurs. day. ,. . De...

M51/NGC5194

M51/NGC5194

  • tatyana-admore
  • 13 Slides

The Whirlpool Galaxy. Marcus Fodor. Why I chose M...

Chapter 23 The Milky Way Galaxy

Chapter 23 The Milky Way Galaxy

  • briana-ranney
  • 46 Slides

23.1 Our Parent Galaxy. 23.2 Measuring the Milky ...

Disk Galaxies – Including the Milky Way.

Disk Galaxies – Including the Milky Way.

  • natalia-silvester
  • 45 Slides

M51 – A typical spiral-disk galaxy. The M81 gro...

What Shapes Galaxies?

What Shapes Galaxies?

  • tatiana-dople
  • 30 Slides

STScI. , 27 April 2016 . Anne-Marie Weijmans. Uni...

ChIP

ChIP

  • faustina-dinatale
  • 35 Slides

- . Seq. Peak Calling in Galaxy. Lisa Stubbs. Ch...

Astronomy 170:

Astronomy 170:

  • alexa-scheidler
  • 27 Slides

Aug. 24 -- 10am class. Turn in HW 1 in the fron...

Many galaxies have powerful energy sources in their nuclei

Many galaxies have powerful energy sources in their nuclei

  • celsa-spraggs
  • 80 Slides

These are called . active. . galaxies. .. . Act...

c omputational

c omputational

  • briana-ranney
  • 34 Slides

a. strophysics (@ . Uchicago. ) in 2042. http://....

Galaxy feedback in 3D

Galaxy feedback in 3D

  • mitsue-stanley
  • 37 Slides

Roberto Maiolino. Feedback is the key:. - reduci...

Galaxy Evolution and Environment (Malaysia, 03/04/2009)

Galaxy Evolution and Environment (Malaysia, 03/04/2009)

  • alida-meadow
  • 26 Slides

Build-up of the red sequence of galaxies thr...

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