Observing Secular Evolution in Distant Galaxies - 2
Not Available
Scoville, N.
Advertised on:
11
2011
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Observing Secular Evolution in Distant Galaxies - 3Not AvailableScoville, N.
Advertised on:
112011 -
Observing Secular Evolution in Distant Galaxies - 4Not AvailableScoville, N.
Advertised on:
112011 -
Observing the Dark Matter Density Profile of Isolated GalaxiesUsing the Sloan Digital Sky Survey (SDSS), we probe the halo mass distribution by studying the velocities of satellites orbiting isolated galaxies. In a subsample that covers 2500 deg2 on the sky, we detect about 3000 satellites with absolute blue magnitudes going down to MB=-14; most of the satellites have MB=-16 to -18, comparable to thePrada, Francisco et al.
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112003 -
OJ 287IAUC 6104 available at Central Bureau for Astronomical Telegrams. IAUC 6104 available at Central Bureau for Astronomical Telegrams.Fiorucci, M. et al.
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111994 -
Old Main-Sequence Turnoff Photometry in the Small Magellanic Cloud. II. Star Formation History and its Spatial GradientsWe present a quantitative analysis of the star formation history (SFH) of 12 fields in the Small Magellanic Cloud (SMC) based on unprecedented deep [(B - R), R] color-magnitude diagrams (CMDs). Our fields reach down to the oldest main-sequence turnoff with a high photometric accuracy, which is vital for obtaining accurate SFHs, particularly atNoël, Noelia E. D. et al.
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112009