13 Dalcanton PPTs View free & download

Dr. Julianne Dalcanton (University of Washington) PowerPoint PPT Presentation

Dr. Julianne Dalcanton (University of Washington) - Multi Cycle Treasury Program

Multi Cycle Treasury Program

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On the other hand .... PowerPoint PPT Presentation

On the other hand .... - On the other hand .... CDM simulations consistently produce halos that are cusped at the center. This has been known since the 1980 s, and has been popularized by ...

On the other hand .... CDM simulations consistently produce halos that are cusped at the center. This has been known since the 1980 s, and has been popularized by ...

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Recent Star Formation Histories of Dwarf Galaxies PowerPoint PPT Presentation

Recent Star Formation Histories of Dwarf Galaxies - Recent Star Formation Histories of Dwarf Galaxies. Evan Skillman U. ... 2 HST WFPC2 GO Programs -- 11 papers on studies of nearby dwarf galaxies ... Prelude: ...

Recent Star Formation Histories of Dwarf Galaxies. Evan Skillman U. ... 2 HST WFPC2 GO Programs -- 11 papers on studies of nearby dwarf galaxies ... Prelude: ...

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Studying the Atomic-Molecular Transition in the Local Group PowerPoint PPT Presentation

Studying the Atomic-Molecular Transition in the Local Group - Studying the Atomic-Molecular Transition in the Local Group. Erik Rosolowsky ... Wong & Blitz (2002) studied CO and star formation in a sample of 7 galaxies. ...

Studying the Atomic-Molecular Transition in the Local Group. Erik Rosolowsky ... Wong & Blitz (2002) studied CO and star formation in a sample of 7 galaxies. ...

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Clues to Nuclear Star Cluster Formation from Edge-on Galaxies PowerPoint PPT Presentation

Clues to Nuclear Star Cluster Formation from Edge-on Galaxies - Clues to Nuclear Star Cluster Formation from. Edge-on Galaxies. Anil Seth (U. of ... Spheroid vs. Disk color difference: 0.3-0.6 mags, implies disk age 1 Gyr ...

Clues to Nuclear Star Cluster Formation from. Edge-on Galaxies. Anil Seth (U. of ... Spheroid vs. Disk color difference: 0.3-0.6 mags, implies disk age 1 Gyr ...

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OIR national facilities roadmap PowerPoint PPT Presentation

OIR national facilities roadmap - Alan Dressler, Carnegie Observatories; National Research Council, Astronomy and ... Michael A. Strauss, Princeton University; Chair, LSST Science Working Group ...

Alan Dressler, Carnegie Observatories; National Research Council, Astronomy and ... Michael A. Strauss, Princeton University; Chair, LSST Science Working Group ...

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HWR - 1/3 of all stars at z~0 are in disks ... than the na ve halo-scalings lead. us to expect! H2/3(z) HWR. Princeton, 2005. HWR. Princeton, 2005 ...

1/3 of all stars at z~0 are in disks ... than the na ve halo-scalings lead. us to expect! H2/3(z) HWR. Princeton, 2005. HWR. Princeton, 2005 ...

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Signatures of CDM substructure in tidal debris PowerPoint PPT Presentation

Signatures of CDM substructure in tidal debris - Signatures of ?CDM substructure in tidal debris. Jennifer Siegal-Gaskins ... Dwarf galaxies may already be too dispersed in Lz to see effect of substructure ...

Signatures of ?CDM substructure in tidal debris. Jennifer Siegal-Gaskins ... Dwarf galaxies may already be too dispersed in Lz to see effect of substructure ...

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THE UNIVERSE: FROM PARTICLES TO GALAXIES - THE UNIVERSE: FROM PARTICLES TO GALAXIES

THE UNIVERSE: FROM PARTICLES TO GALAXIES

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Stellar population properties of bulges PowerPoint PPT Presentation

Stellar population properties of bulges - Proctor & Sansom (2002, MNRAS) 32 objects (11 Es, 6 S0s, 16 bulges) ... Proctor, Sansom, Reid, 2000. Stellar Population Gradients. Mehlert, Thomas et al. 2003 ...

Proctor & Sansom (2002, MNRAS) 32 objects (11 Es, 6 S0s, 16 bulges) ... Proctor, Sansom, Reid, 2000. Stellar Population Gradients. Mehlert, Thomas et al. 2003 ...

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On the other hand .... - a cored halo gives a solid body rotation curve near the ... The halo density profiles can also be used to derive constraints ... the baryons to the dark halo ...

a cored halo gives a solid body rotation curve near the ... The halo density profiles can also be used to derive constraints ... the baryons to the dark halo ...

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The LuminositySize relation of galaxies PowerPoint PPT Presentation

The LuminositySize relation of galaxies - Spheroids (inc bulges) and discs are fundamentally different ... in bulges 50% in ... big issue (bulges heavily attenuated) disks 0.2-1.1 mag, bulges: 0.8 ...

Spheroids (inc bulges) and discs are fundamentally different ... in bulges 50% in ... big issue (bulges heavily attenuated) disks 0.2-1.1 mag, bulges: 0.8 ...

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Dynamics of substructures: On survivors and debris PowerPoint PPT Presentation

Dynamics of substructures: On survivors and debris - If radial and constant anisotropy: too fastly rising dispersion near the centre, ... the anisotropy has to be tangential. This is why NFW profiles require 0 ...

If radial and constant anisotropy: too fastly rising dispersion near the centre, ... the anisotropy has to be tangential. This is why NFW profiles require 0 ...

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Dalcanton PowerPoint PPT Presentations