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Milky Galaxies published presentations and documents on DocSlides.

EDUCATIONAL

EDUCATIONAL

  • danika-pritchard
  • 27 Slides

RESEARCH. q. uality and quantity. Paul Dowling. I...

Measuring Distances

Measuring Distances

  • tawny-fly
  • 25 Slides

Introduction. Trigonometric Parallax . Spectrosco...

Deciphering the CIB

Deciphering the CIB

  • conchita-marotz
  • 40 Slides

12 Oct 2012. Banyuls. MODELING COUNTS AND CIBA WI...

SDSS Quasar Science

SDSS Quasar Science

  • calandra-battersby
  • 45 Slides

With thanks to the members of the Quasar Working ...

Grand unification of AGN activity across the universe

Grand unification of AGN activity across the universe

  • celsa-spraggs
  • 23 Slides

Nikos Fanidakis. and. C.M. Baugh, R.G. Bower, S. ...

Q1: Quenching and the cessation of star-formation

Q1: Quenching and the cessation of star-formation

  • ellena-manuel
  • 17 Slides

1. The ". Q". word and its meaning. Is quenching...

Elizabeth J. McGrath, Aurora Y.

Elizabeth J. McGrath, Aurora Y.

  • faustina-dinatale
  • 20 Slides

Kesseli. , . Arjen. van der . Wel. , Eric Bell, ...

Keck spectroscopy and dynamical masses for a large sample o

Keck spectroscopy and dynamical masses for a large sample o

  • mitsue-stanley
  • 27 Slides

1 < z < 1.6 passive red galaxies. Sirio Bel...

Connecting Warm H

Connecting Warm H

  • natalia-silvester
  • 48 Slides

2. Emission and Active Transformation within Com...

The relative size of the Universe

The relative size of the Universe

  • liane-varnes
  • 18 Slides

1.6093. 1. DISTANCE. km. miles. LY (Light years)....

X-Shaped Radio Galaxies and the Gravitational Wave Backgrou

X-Shaped Radio Galaxies and the Gravitational Wave Backgrou

  • jane-oiler
  • 51 Slides

David Roberts, Jake Cohen, & Jing Lu. Brandei...

Double Trouble: ASKAP Early Science using Radio Galaxies

Double Trouble: ASKAP Early Science using Radio Galaxies

  • pamella-moone
  • 17 Slides

Lawrence Rudnick, University of Minnesota. Deep+w...

Radio Mode Feedback in Giant Elliptical Galaxies

Radio Mode Feedback in Giant Elliptical Galaxies

  • faustina-dinatale
  • 20 Slides

Paul . Nulsen. (. CfA. ), Christine Jones (. CfA...

USING LOW

USING LOW

  • marina-yarberry
  • 33 Slides

POWER . RADIO. GALAXIES AS BEACONS FOR CLUSTERS ...

Fraction of galaxies of different types plotted as function

Fraction of galaxies of different types plotted as function

  • yoshiko-marsland
  • 25 Slides

Galaxy Morphology and Environment. Main relation ...

Astronomy 1 –

Astronomy 1 –

  • debby-jeon
  • 70 Slides

Fall 2014. Lecture . 16; December 8, 2014. Previ...

Do your course evaluations.

Do your course evaluations.

  • natalia-silvester
  • 39 Slides

http://www.pa.uky.edu. I will add 5 points on you...

Astronomy 1 –

Astronomy 1 –

  • luanne-stotts
  • 63 Slides

Fall 2014. . Lecture . 15; December 4, . 2014. P...

The Stellar Populations of Galaxies

The Stellar Populations of Galaxies

  • yoshiko-marsland
  • 18 Slides

H.-W. Rix IMPRS Galaxies Course March 11, 2011....

Gravitational

Gravitational

  • myesha-ticknor
  • 43 Slides

Redshift. in Clusters of Galaxies. Marton Trencse...

Back to the Beginning: Big Bang

Back to the Beginning: Big Bang

  • stefany-barnette
  • 34 Slides

. Misnomer. ! . . Expansion not explosion. No c...

Stellar-mass

Stellar-mass

  • mitsue-stanley
  • 23 Slides

Metallicity. Relation at High . Redshifts. Stell...

The Doppler Effect

The Doppler Effect

  • lois-ondreau
  • 10 Slides

, and Red-Shifts. The Doppler Effect. http://www....

GRBs as cosmological probes

GRBs as cosmological probes

  • lois-ondreau
  • 33 Slides

Thomas Krühler (DARK). Thanks to J. . Fynbo. , D...

physicsweb.orglook deep into the universe,wesee stars and galaxies ofa

physicsweb.orglook deep into the universe,wesee stars and galaxies ofa

  • trish-goza
  • 100 Slides

           ...

Hubble Diagram: Distribution of Galaxies

Hubble Diagram: Distribution of Galaxies

  • faustina-dinatale
  • 14 Slides

Hubble’s Law: v = H. o. d. Velocity increases w...

Quantum vacuum and the gravitational repulsion between matt

Quantum vacuum and the gravitational repulsion between matt

  • trish-goza
  • 25 Slides

D.S. . Hajdukovic. GBAR Collaboration Meeting. 18...

Chemo-dynamics of galaxies with resolved stellar population

Chemo-dynamics of galaxies with resolved stellar population

  • danika-pritchard
  • 21 Slides

Giuseppina. . Battaglia. Instituto. de . Astrof...

TWO DIVINE REVELATIONS

TWO DIVINE REVELATIONS

  • lois-ondreau
  • 131 Slides

The Bible. The Record of Nature. Written. Specifi...

Vocabularies in the VO

Vocabularies in the VO

  • tatyana-admore
  • 29 Slides

Alasdair J G Gray. Norman Gray. Iadh. . Ounis. W...

The Explicator Project:

The Explicator Project:

  • debby-jeon
  • 59 Slides

. Integrating Astronomy Data with Semantic Web T...

University

University

  • luanne-stotts
  • 37 Slides

of Arizona (. UofA. ). SHARDS: An unbiased . spec...

A Galaxy Revealed in Multiple Wavelengths

A Galaxy Revealed in Multiple Wavelengths

  • conchita-marotz
  • 16 Slides

0. Topic: . Multiwavelength observations. Concept...

Pauline Gagnon

Pauline Gagnon

  • test
  • 25 Slides

Physicist and communicator at CERN. The dark side...

!At z ~ 0, at least 30% of all galaxies show some sign of a nuclear ac

!At z ~ 0, at least 30% of all galaxies show some sign of a nuclear ac

  • stefany-barnette
  • 100 Slides

s) and optically violently variable (OVV) objects!

Cosmic

Cosmic

  • sherrill-nordquist
  • 41 Slides

. Reionization. . . Chris . Carilli. (. M/N. ...

1 On star-formation compactness & bulges: the ALMA view

1 On star-formation compactness & bulges: the ALMA view

  • celsa-spraggs
  • 5 Slides

S. IR. (z~2) = . S. IR. (z~0) x 6. S. IR. (z~4) =...

Synchrotron Radiation,

Synchrotron Radiation,

  • debby-jeon
  • 45 Slides

continued. Rybicki. & . Lightman. Chapter 6...

The Origin of Stars

The Origin of Stars

  • cheryl-pisano
  • 64 Slides

Christopher W. Ashcraft M.S., M.Ed.. Big Bang vs...

High-

High-

  • alexa-scheidler
  • 21 Slides

Redshift. Galaxies . in Cluster Fields. Wei Zhen...

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