Schmidt (1959) speculated that the star formation rate is proportional to a power
of the surface density of the interstellar medium
 |
(3.1) |
where the power
seems between 1 and 2 around the solar vicinity.
If
, the star formation rate is thought to be determined by the collision rate
of interstellar clouds.
At that time Schmidt showed us
.
On the other hand, if the gas passing through the galactic arms forms stars,
the star formation rate seems proportional to the gas surface density and the arm-to-arm
period.
Thus this predicts
.
Subsections
Kohji Tomisaka
2009-12-10