Search Results for 'Galaxies Galaxy'

Galaxies Galaxy published presentations and documents on DocSlides.

Radio Mode Feedback in Giant Elliptical Galaxies
Radio Mode Feedback in Giant Elliptical Galaxies
by faustina-dinatale
Paul . Nulsen. (. CfA. ), Christine Jones (. CfA...
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...
Radio Mode Feedback in Giant Elliptical Galaxies
Radio Mode Feedback in Giant Elliptical Galaxies
by celsa-spraggs
Paul . Nulsen. (. CfA. ), Christine Jones (. CfA...
Stellar populations in disc galaxies from the CALIFA survey
Stellar populations in disc galaxies from the CALIFA survey
by luanne-stotts
Patricia . Sánchez-Blázquez. (UAM). Jairo. Me...
Active Galaxies
Active Galaxies
by olivia-moreira
Lesson Objectives. To appreciate that some galaxi...
Dust in Dwarf Galaxies
Dust in Dwarf Galaxies
by ellena-manuel
Adam Leroy. National Radio Astronomy Observatory....
Hot Gas in Elliptical and BCG Galaxies
Hot Gas in Elliptical and BCG Galaxies
by min-jolicoeur
Craig Sarazin. University of Virginia. M86. (. Ra...
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...
Stars, Galaxies, and the Universe
Stars, Galaxies, and the Universe
by pasty-toler
Chapter 2. Stars. Section 1 Vocabulary. Spectrum....
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...
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...
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 ...
Q1: Quenching and the cessation of star-formation
Q1: Quenching and the cessation of star-formation
by ellena-manuel
1. The ". Q". word and its meaning. Is quenching...
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...
Connecting Warm H
Connecting Warm H
by natalia-silvester
2. Emission and Active Transformation within Com...
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...
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...
The ISM structure of low-
The ISM structure of low-
by conchita-marotz
metallicity. star-forming dwarf galaxies. Diane...
Formation of the Hubble Sequence
Formation of the Hubble Sequence
by marina-yarberry
Michael Fall. STScI. . CoolSci. Talk. ...
Faint
Faint
by olivia-moreira
Dwarf Galaxies in . Fornax. . Shed . Light on a ...
USING LOW
USING LOW
by myesha-ticknor
POWER . RADIO. GALAXIES AS BEACONS FOR CLUSTERS ....
Detection of H-alpha emission from
Detection of H-alpha emission from
by myesha-ticknor
z. >3.5 galaxies with. AKARI-FUHYU NIR spectro...
Astrophysics from Space
Astrophysics from Space
by phoebe-click
Lecture 8: Dusty starburst galaxies. Prof.. . Dr...
Pseudo-bulges, classical bulges and
Pseudo-bulges, classical bulges and
by phoebe-click
elliptical galaxies – II. Monsters at Heart. Di...
Fitting
Fitting
by pasty-toler
the full SED (. from. UV to . far-IR. ) of gala...
Herschel observations: contraints on
Herschel observations: contraints on
by myesha-ticknor
dust. . attenuation. and star formation histori...
Alexandra Pope (UMass Amherst)
Alexandra Pope (UMass Amherst)
by calandra-battersby
JWST Workshop. – . STScI. Baltimore. June 8, ...
Chapter 14
Chapter 14
by kittie-lecroy
Modern Cosmology. Look at your thumb.. The matter...
The Detectability of Lyα Emission from Galaxies during
The Detectability of Lyα Emission from Galaxies during
by olivia-moreira
the Epoch of Reionization. Dijkstra. , . Mesinger...
DYNAMO Survey:
DYNAMO Survey:
by debby-jeon
An up-close view of turbulent, clumpy galaxies. ...
Tsutomu T. TAKEUCHI
Tsutomu T. TAKEUCHI
by tatyana-admore
Division of Particle and Astrophysical Science, N...