Astro 1050 Fri. Mar 26, 2004
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Today: Astronomy Articles |
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End Ch. 12: The Milky Way |
The Galactic Rotation
Curve
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Keplerian fall-off near center
indicates compact mass at center |
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Flat curve throughout disk indicates
much distributed mass |
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Lack of fall-off beyond visible “edge”
indicates “dark matter” |
Stellar Population and
Galaxy Evolution
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“Metal” abundance during time |
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“Metals” are elements heavier than He |
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A given star’s atmospheric abundance is
approx. fixed at birth |
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Interstellar metal abundance grows with
each new generation of stars |
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Red giants and supernova eject new
heavy elements into interstellar gas |
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Orbits during time |
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A given star’s orbit is approx. fixed
at birth – just plows through gas |
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Orbits of gas clouds evolve with time
since they can collide |
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Orbits get more circular and disk-like
with time |
Traditional Model of
Galaxy Evolution
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Stars are stuck with their original
orbits |
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They plow through gas like bullets |
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Orbits of gas can evolve |
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Gas clouds collide and only average
motion (rotation) survives |
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Metal abundance grows with time |
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System starts out with little organized
motion,few metals |
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Halo stars form at this time |
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It contracts, velocities average out
leaving only rotation |
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Gas collapses to form the disk |
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Disk stars form after this has happened |
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Some problems with traditional model |
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Globular clusters not all same age |
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Gap in ages between halo and disk
objects |
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Presence of some metals in even in
oldest stars |
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System may have formed by merger of
smaller galaxies |
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Galactic Cannibalism |
M51: The Whirlpool Galaxy
Possible Origin of Spiral
Arms
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Differential rotation smears features
out into spiral patterns |
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But can’t be whole story: |
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Number of times Sun has orbited the
galaxy: |
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10 billion yr/200 million yr
= 50 times |
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Spiral arms would have been wound up
very tightly |
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Something must continuously rebuild
them |
Degree of
Organization
of the Spiral Arms
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Different degrees of organization |
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Grand Design
Spirals: M51 |
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Flocculent (“wooly”) Spirals |
Degree of
Organization
of the Spiral Arms
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Different degrees of organization |
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Grand Design
Spirals: M51 |
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Flocculent (“wooly”) Spirals |
Tracing the Spiral Arms
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Arms NOT obvious if you look at: |
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Old objects like the sun |
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Arms ARE obvious if you look at: |
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Maps of gas clouds |
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21 cm Hydrogen |
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Radio maps of CO |
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Far infrared observations of dust |
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Young stars |
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O, B stars |
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“HII” ionized hydrogen regions
surrounding O,B stars |
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Clouds somehow form in arms , then
dissipate between them |
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Short lived objects only get a short
distance from their places of birth |
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O stars, Lifetime = few million
years, at 250 km/s Þ500 pc |
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M51: The Whirlpool Galaxy
Density Wave Theory
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SPIRAL WAVE rotates with galaxy, but
slower than individual stars |
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Like moving traffic jam after an
accident has been cleared |
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Gas (and stars) catch up with wave,
move through it, eventually reach front |
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Just like cars catching up with moving
traffic jam, eventually get through it |
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Gas is more crowded in wave – clouds
collapse to form new stars |
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More collisions in the traffic jam |
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There are slightly more old stars in
the arm too, because they speed up slightly coming into it and slow down
slightly moving out of it. |
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But the best tracers are the things
that mark recent cloud collapses: O,B
stars, etc. |
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Self Sustaining Star
Formation
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Cloud collapse Þ New stars |
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New stars Þ Supernova after few
million years |
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Supernova Þ Shock Waves |
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Shock Waves Þ Nearby clouds collapse |
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Differential Rotation twists pattern
into spiral |
Two limiting cases of
spirals
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Grand Design: Density Wave |
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Flocculent: Self Sust. Star Form. +
Diff. Rot. |
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In most Galaxies you have some
combination of the two |
The Nucleus of the Galaxy
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Likely Black hole |
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High velocities |
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Large energy generation |
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At
a=275 AU P=2.8 yr Þ 2.7 million
solar masses |
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Radio image of Sgr A
about 3 pc across, with model of surrounding disk |
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A movie of stars at the
core
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www.mpe.mpg.de/www_ir/GC |
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Very cool, and worth a look! |
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This is the best evidence to date for a
massive black hole at the Galactic core.
Now essentially “proven.” |