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Galaxies Gas published presentations and documents on DocSlides.

From the Galaxy to galaxies: star clusters as probes of the formation and evolution of galaxies ove
From the Galaxy to galaxies: star clusters as probes of the formation and evolution of galaxies ove
by maniakiali
Laura . Magrini. INAF- . Osservatorio. . Astrofis...
X-Shaped Radio Galaxies and the Gravitational Wave Backgrou
X-Shaped Radio Galaxies and the Gravitational Wave Backgrou
by jane-oiler
David Roberts, Jake Cohen, & Jing Lu. Brandei...
The Stellar Populations of Galaxies
The Stellar Populations of Galaxies
by yoshiko-marsland
H.-W. Rix IMPRS Galaxies Course March 11, 2011....
Chemo-dynamics of galaxies with resolved stellar population
Chemo-dynamics of galaxies with resolved stellar population
by danika-pritchard
Giuseppina. . Battaglia. Instituto. de . Astrof...
Nearby Galaxies: What Next?
Nearby Galaxies: What Next?
by yoshiko-marsland
D. Calzetti (Univ. of Massachusetts). a. nd the L...
The Milky Way and Other Galaxies
The Milky Way and Other Galaxies
by tawny-fly
Recap. Canvas homework: due on Wednesday. Lab thi...
Galaxies and the Universe
Galaxies and the Universe
by tatyana-admore
The Milky Way Galaxy. When you look into the hazy...
Clusters of galaxies
Clusters of galaxies
by giovanna-bartolotta
With a wide-field multi-IFU spectrograph. Cluster...
Observations of the evolution of HI in galaxies across diff
Observations of the evolution of HI in galaxies across diff
by tatiana-dople
D.J. Pisano. (West Virginia University). Why stud...
The cosmological formation of massive galaxies
The cosmological formation of massive galaxies
by ellena-manuel
Thorsten Naab . MPA, . Garching. . What regulate...
How special are brightest group and cluster galaxies?
How special are brightest group and cluster galaxies?
by tawny-fly
Anja. von . der. Linden et al., 2007, MNRAS, 3...
Active Galaxies
Active Galaxies
by olivia-moreira
Lesson Objectives. To appreciate that some galaxi...
Interactions Between Galaxies
Interactions Between Galaxies
by olivia-moreira
. Loners. Interactions were once . believed to...
Determining broad-band spectra of radio galaxies with the EVLA
Determining broad-band spectra of radio galaxies with the EVLA
by briana-ranney
Jeremy . Harwood. YERAC 2011. Background Image co...
SOAR 2018: Galaxies Aileen A. O’Donoghue
SOAR 2018: Galaxies Aileen A. O’Donoghue
by faustina-dinatale
Priest Associate Professor of Physics. Galaxies. ...
Chapter 16 A Universe of Galaxies
Chapter 16 A Universe of Galaxies
by calandra-battersby
The Hubble Deep Field. 10 day exposure –field l...
Understanding Local Luminous Infrared Galaxies in the
Understanding Local Luminous Infrared Galaxies in the
by stefany-barnette
Herschel. Era. Jason K. . Chu (jasonchu@. ifa.ha...
The Slit-Less Spectroscopic Survey of Galaxies (SPICY) with
The Slit-Less Spectroscopic Survey of Galaxies (SPICY) with
by collectmcdonalds
AKARI/IRC – perspective to SPICA. T. . Wada, . Y...
The Universe Motions of galaxies
The Universe Motions of galaxies
by ani
The expanding Universe. Recap. Milky . Way. Distan...
Measuring Distances to Galaxies Using
Measuring Distances to Galaxies Using
by williams
Water Vapor . Megamasers. Jim Braatz (NRAO). Measu...
The Lyman Continuum Escape
The Lyman Continuum Escape
by yoshiko-marsland
Fraction. Harry . Teplitz. ,. Brian . Siana. , &a...
Millennium Data Dissemination
Millennium Data Dissemination
by pasty-toler
2012-11-26. MPA institute seminar. 1. possible ex...
Robert Foot,
Robert Foot,
by phoebe-click
CoEPP. , University . of Melbourne. June . 26 201...
Astro-2: History of the Universe
Astro-2: History of the Universe
by lois-ondreau
Lecture 3; April . 11 2013. Previously.. On Astro...
Gravitational Lensing
Gravitational Lensing
by tawny-fly
Boot Camp. Robert Nemiroff. Michigan Tech . Abstr...
Gravitational Lensing
Gravitational Lensing
by cheryl-pisano
and. Quasars . “A man should look for what is, ...
Astro
Astro
by alexa-scheidler
101 Slide Set: Finding . the Most Luminous Galax...
ASKAP Continuum
ASKAP Continuum
by test
S. urveys . of . Local Galaxies. Michael . Brown....
Measuring Distances
Measuring Distances
by tawny-fly
Introduction. Trigonometric Parallax . Spectrosco...
Deciphering the CIB
Deciphering the CIB
by conchita-marotz
12 Oct 2012. Banyuls. MODELING COUNTS AND CIBA WI...
USING LOW
USING LOW
by marina-yarberry
POWER . RADIO. GALAXIES AS BEACONS FOR CLUSTERS ...
Elizabeth J. McGrath, Aurora Y.
Elizabeth J. McGrath, Aurora Y.
by faustina-dinatale
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
by mitsue-stanley
1 < z < 1.6 passive red galaxies. Sirio Bel...
Double Trouble: ASKAP Early Science using Radio Galaxies
Double Trouble: ASKAP Early Science using Radio Galaxies
by pamella-moone
Lawrence Rudnick, University of Minnesota. Deep+w...
Astronomy 1 –
Astronomy 1 –
by debby-jeon
Fall 2014. Lecture . 16; December 8, 2014. Previ...
Do your course evaluations.
Do your course evaluations.
by natalia-silvester
http://www.pa.uky.edu. I will add 5 points on you...
Hubble Diagram: Distribution of Galaxies
Hubble Diagram: Distribution of Galaxies
by faustina-dinatale
Hubble’s Law: v = H. o. d. Velocity increases w...
University
University
by luanne-stotts
of Arizona (. UofA. ). SHARDS: An unbiased . spec...
Pauline Gagnon
Pauline Gagnon
by test
Physicist and communicator at CERN. The dark side...
High-
High-
by alexa-scheidler
Redshift. Galaxies . in Cluster Fields. Wei Zhen...