15-01 The Milky Way


  • the shape of the Milky Way
     


    Herschel, around 1800; Kapteyn, around 1900; counting stars
    -- the 'grindstone' model, a disk about 15 kpc in diameter, the Sun is at the center



    [interstellar extinction -- the grindstone model actually counted only nearby stars]

    Harlow Shapley, in 1920, determining distribution of globular clusters
    (using RR Lyrae stars)



    -- the galactic center is in the direction of Sagittarius;
        the Sun is about 8 kpc away from the center!



     
  • dust and stars
    dust, about 10 K - 100 K, radiating in 30 - 300 microns (far infrared)
    stars brighter than dust in near infrared (< 10 microns); extinction in this band not severe
    dust in the disk, many stars concentrated near the nucleus of the Milky Way



     
  • the three components of our Milky Way galaxy



    disk: dust; young, metal-rich, population I stars
    halo: old, metal-poor, population II stars; 1% of these stars are in globular clusters
    central bulge: containing both population I and population II stars