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Milky Way: Galactic Structure and Dynamics

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... Pulsating Cepheid, RR Lyrae Stars Apparent Magnitude (m) vs. T(d) Shape and Constituents of the Galaxy Most of the matter in the Galaxy is not visible ... – PowerPoint PPT presentation

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Title: Milky Way: Galactic Structure and Dynamics


1
Milky WayGalactic Structure and Dynamics
  • Milky Way has spiral structure
  • Galactic Bulge surrounds the Center
  • Powerful radio source Sagittarius A at Center
  • Contains Super-Massive Black Hole
  • M(SMBH) 106 M(Sun)

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Milky Way Bright Band Across Sky(Resolved by
Galileo)
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Milky Way Galactic Structure
7
Our Galaxy Milky Way
  • Spiral galaxy, e.g. Milky way, Andromeda
  • Sun is located in the disk, but far away from
    the center, about 8000 parsecs (1 pc 3.28 LY)
  • MW appears as a bright band across the sky
  • Determine the size of the galaxy from RR Lyrae
    stars in globular clusters that lie above the
    plane of the galaxy (a globular cluster has about
    a million stars)
  • Period-Luminosity relation for Cepheid variables
    and RR Lyrae gives the magnitude M of absolute
    luminosity L
  • Distance modulus relation relates the magnitude
    m of the apparent luminosity to distance d at 10
    pc
  • m M 5 log (d/10)

8
Shape and Constituents of the Galaxy
  • Most of the matter in the Galaxy is not visible
    (at visible wavelengths)
  • But observations in other wavelength ranges,
    such as the IR and Radio reveal most of the
    matter
  • Matter too cold to emit shorter wavelength
    radiation
  • Spiral arms have hot O and B stars, with ionized
    H II regions, but interstellar matter is
    molecular H2 or atomic H I
  • H I is traced by a hyper-fine structure
    transition due to magnetic interaction between
    spins of the electron and the proton, at radio
    wavelength 21 cm

9
The Hydrogen 21-cm radio map of the Sky and the
Galaxy
10
H I 21 cm Hyperfine Transition
11
Keplers 2nd law velocity varies inversely with
distance from center 3rd Law P2 a3 ? longer
period at larger distance lower velocity
12
Mass, Velocity, Radius of a Galaxy
  • Mass at radius R has rotational velocity given
    by this relation
  • Rotational velocity should decrease with R,
    since M should
  • decrease with R

13
Measuring Rotational Velocities Doppler Effect
14
Measure velocities using Doppler Effect
15
Dark Matter
  • Why are rotational velocities constant, in
    violation of Keplers laws for gravitationally
    bound orbits ?
  • The Suns period P around the center of MW is
    related to the mass inside the Suns orbit (mass
    outside should have no effect on Keplers Laws)
  • If the rotational velocity of matter (H I) is
    the same in the outer regions of the galaxy, then
    there must be unseen matter outside the Suns
    orbit Dark Matter !
  • Estimates indicate more than 90 is Dark Matter
    (as much dark matter as visible). NO CLUE !!!

16
Galactic StructureSpiral Arms Density Waves
  • Spiral arms made of stars, dust, and gas should
    dissipate after some time, arms should unwind
  • But they maintain a stationary pattern like the
    spokes on a wheel
  • Gravitational density waves through galactic
    matter, propagating like water waves matter
    itself is not dislocated after the wave
    disturbance passes (periodically)
  • Concentration of matter in spiral arms leads to
    formation of massive O,B stars that are
    short-lived

17
Galactic Dynamics and Spiral Structure
18
Slower traffic creates gaps
19
Stellar Populations and Ages
  • Population I (Pop I) metal-rich, young,
    massive, bright stars found in the spiral arms,
    e.g. Cepheid variables (metals all elements
    besides H, He) the Sun is an intermediate Pop
    I star
  • Pop II old, metal-poor stars found in the halo
    and globular clusters above the plane of the
    galaxy (e.g. RR Lyrae stars)
  • The Bulge of the galaxy has a mixture of Pop I
    and Pop II stars
  • Pop III are metal-poor stars in the early
    Universe, predominantly primordial H and He

20
Center of our Galaxy
  • A massive Black Hole ? How do we know ?
  • Extremely luminous, indicating huge
    concentration of interacting matter
  • Observations of stellar orbits around the Center
    must be moving extremely fast ! Can calculate
    mass at the center of the orbit using modified
    Keplers third law

21
Sagittarius A Galactic Center
Radio Source Not visible due to dust extinction
22
Stellar Orbits Around the Sgr A
Keplers laws and Law of gravitation yield
Super-Massive Black Hole mass
23
Mass of the Black Hole at the Center of Milky Way?
Mass enclosed within a volume at a given
distance Mo/pc3
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