Kathryn Johnston

30.06.2013 • Views

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Kathryn Johnston

Kathryn Johnston

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Boxsize:<br />

300kpc<br />

38-23<br />

mag/arcsec^2<br />

-2.5 < [Fe/H]<br />

< -0.5<br />

-0.1 < [alpha/Fe]<br />

< 0.2

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What is different about LINER Galaxies

Stephen Murray - Astronomy and Astrophysics - University of ...

UCSC Astronomy & Astrophysics Orientation Guide last update ...

Astronomy 1: Introduction to the Cosmos, Winter 2013, UCSC

Light, Optics and Telescopes Trip to Lick Observatory

Frank van den Bosch

Jason X. Prochaska

Leo Blitz

Risa Wechsler - Astronomy and Astrophysics

Stéphane Courteau

Kim Griest

Ofer Lahav

Michael Strauss

Laurence Tresse

Boxsize: 300kpc 38-23 mag/arcsec^2 -2.5 < [Fe/H] < -0.5 -0.1 < [alpha/Fe] < 0.2

Abundance Patterns in Satellites vs Halo

Page 1 and 2: Stellar Halos and Satellite Systems
Page 3 and 4: Dark matter modeled via merger tree
Page 5 and 6: Model for Formation of a Halo Color
Page 7 and 8: Features brighter than 30 mag/ arcs
Page 9 and 10: Model for Formation of a Halo - Hal
Page 11 and 12: Abundance Patterns in Satellites vs
Page 13: Abundance Patterns in Satellites vs
Page 17 and 18: ... only stars with [alpha/ Fe]