Astronomical Applications Department, U.S. Naval Observatory thesis Page 9
List
of
T
ables
1.1 Adopted Parameters for Holmberg II . . . . . . . . . . . . . . . .
8
1.2 Adopted Parameters for IC2574 . . . . . . . . . . . . . . . . . . .
9
1.3 Adopted Parameters for Sextans A . . . . . . . . . . . . . . . . . 11
2.1 UIT Observations . . . . . . . . . . . . . . . . . . . . . . . . . . 18
2.2 Optical Observations . . . . . . . . . . . . . . . . . . . . . . . . . 20
3.1 Integrated Magnitudes . . . . . . . . . . . . . . . . . . . . . . . . 25
4.1 Peak FUV Surface Brightness in Relation to Galaxy Center . . . . 38
4.2 Star Formation Rates from Observed Luminosities . . . . . . . . . 46
4.3 Star Formation Rates from Corrected Luminosities . . . . . . . . 47
4.4 Normalized Star Formation Rates and Gas Properties . . . . . . . 49
5.1 Derived Properties of Star Forming Regions . . . . . . . . . . . . 61
7.1 Derived Properties of Clusters in HI holes . . . . . . . . . . . . . 101
viii