Evolution of isolated neutron stars: young coolers and old accretors Sergei Popov (SAI)
Neutron stars - Chapter 21 1. Neutron stars The remains of cores of some massive stars that have become supernovae. Cores are a degenerate gas of mostly.
Http://constellation.nasa.gov Beyond Einstein: From the Big Bang to Black Holes Neutron Star Fundamental Physics with Constellation-X ~ 1 x 10 15 g cm.
Searching for gravitational waves with lasers Rick Savage Caltech LIGO Hanford Observatory - Richland, WA.
Intro X-rays From the Sky Chandra X-ray Observatory November, 2003.
A Few Ways of Acquiring Telescope Time Telescope Committee Astronomical Society of New York October 23, 2009 Peter Wehinger Steward Observatory University.
Microwave: The Cosmic Microwave Background (CMB). Shortly after the Big Bang, the Universe cooled enough to allow atoms to form. After this point in time,
DOE Review (June 3, 2004) PoGO by T.Kamae 1 Large-Area Balloon-Borne Polarized Gamma Ray Observer (PoGO) DOE Review (June 3, 2004) Tune Kamae for the PoGO.
Announcements Pick up graded homework (projects, tests still in progress) Transit of Mercury (crossing in front of Sun), this afternoon, roughly noon-5:00.
REU TALK – June 14,2011 Signal Processing REU talk 14jun11 Phil Perillat.
Radio Waves Electromagnetic Spectrum Visible Light Waves Microwaves Infrared Waves Ultraviolet Waves X-Ray Waves Gamma Ray Waves.
Science Capabilities - Summary
