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19 Cards in this Set

  • Front
  • Back

Kiloparsec

1,000 PC - 3300 ly (a unit of distance)

Cephic Variable Stars

Stars w/ pulsation of 1-60days. Variation=Luminosity

Instability Strip

Region on H-R diagram. Stars are unstable to pulsation.

Period Luminosity

Relationship of period of pulsation and instinsic brightness

Proper Motion

The rate which a star moves across the sky per arc second

Disk Component

Material confined to the plane of a galaxy

Spherical Component

All the matter in a galaxy in a spherical distribution around the center

Halo

Spherical thing region of galaxy of star material

Central Bulge

The cloud that lies center of spiral galaxy

Rotation Curve

A graph of orbital velocity versus radius

Dark Matter

Nonluminious matter that is detected only by gravitational influence

Spiral Tracer

Objects used to mark the spiral arms

Spiral density wave theory

Spiral arms are compression disk

Self-Sustaining Star Formation

When one star forms more stars

Population 1 Star

Stars with atoms heavier than helium, usually young stars

Population 2 Star

Stars poor in atoms heavier than hellium, older stars

Metal

All atoms heavier than hellium

Monolithic Collapse

A hypothesis that says the galaxy formed from the collapse of a single large cloud of turbulent gas

Sagittarius A

Radio source at core of milky way galaxy