Twenty Years of Microlensing Observations From the Andrzej Udalski Warsaw University Observatory Perspective.
Our Galaxy `. Interstellar dust obscures our view at visible wavelengths along lines of sight that lie in the plane of the galactic disk.
Charles Hakes Fort Lewis College1. Charles Hakes Fort Lewis College2.
Pulsar population overview Dunc Lorimer (WVU) November 2, 2006 The observed sample Spin frequencies > 10 Hz - normal pulsars - recycled objects Current/future.
