Kathryn Mummah What happened before I showed up What you need to know astronomically What I did & the results of my summer at Fermi.

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Presentation transcript:

Kathryn Mummah What happened before I showed up What you need to know astronomically What I did & the results of my summer at Fermi

■ Artists rendition ■ SDSS

 How bright a star looks from Earth  Represented as r0  Backwards scale  Apparent magnitude of the sun is

 Absolute is how bright a star would look if it was 10 pc away ▪ Pc = 3.26 ly = = 19.2 trillion miles ▪ 10 pc = 192 trillion miles  Also a backwards scale  Absolute magnitude of the Sun is 4.83  SCR would have basically the same absolute and apparent

 Color measurement  X-axis goes from blue to red  Y-axis goes from faint to bright  Remember- Backwards scale

WhereHaloThick DiscThin Disc AgeOldest- up to 13.5 GyrIntermediate- > 10 GyrYoungest Gyr Made ofMostly H and HeH and He + some metalH, He, large amount of metal ColorBluestReddest

 Dust makes everything redder  Most dust is assumed to be less than 100 pc from plane  Cobe  Dust map  Measured infrared from plane to 100 pc from plane 100 pc 31,000 pc

 The number of stars above and below the galactic midplane should be the same, because gravity would “smooth out” any large asymmetries

 There is an asymmetry in the number of stars above and below the galactic midplane  400 pc  800 pc Widrow et al ApJ 750, L41 Fractional asymmetry

 Look at the data from the paper “Galactoseismology: Discovery of Vertical Waves in the Galactic Disc” in more detail  Look at color measurements  Break up data into smaller chunks  Figure out if a more detailed paper is needed

1. Dust 2. Satellite Galaxy 3. Dark Matter Halo

 South is redder  How constant  North  South lNorth (G-r) 0 South (G-r) 0 Difference Average Range

 Widrow, Lawrence M., et al. "Galactoseismology: Discovery of Vertical Waves in the Galactic Disc." The Astrophysical Journal Letters (2012): 1-5. The Astrophysical Journal Letters. Web. 20 July /750/2/L41/pdf _750_2_L41.pdf /750/2/L41/pdf _750_2_L41.pdf  Brian Yanny  Chris Stoughton  and his office  George and Kristy  Python  SDSS III data  Logger Pro

1. Dust  Not been properly accounted for  Dust makes things seem farther away ▪ Hidden dust on the bottom ▪ Not comparing equal boxes 2. Different stellar population  Could have come from a satellite galaxy ▪ w/higher Metallicity/ ▪ older population ▪ Passed through bottom  Halo difference (16 kpc)

 M – m = 5 log (d / 10 pc)  M 2 = 40.2 (G-r)