Binary pulsars as tools to study gravity
LIGO-G9900704-v1 Image Processing Pipeline for Follow-up Observations with Optical Telescopes Brenden Simoneaux RET End Summary July 2009.
Pulsar population overview Dunc Lorimer (WVU) November 2, 2006 The observed sample Spin frequencies > 10 Hz - normal pulsars - recycled objects Current/future.
Ya. B. Zeldovich Ya. B. Zeldovich All-Moscow Seminar of Astrophysicists Plamen Fiziev LTF JINR Dubna Models of Neutron Stars without Functional Relation.
Why would you want to know about pulsars and why would you like to discover more?
Neutrino Cooling of Neutron Stars
Ya. B. Zeldovich All-Moscow Seminar of Astrophysicists
Image Processing Pipeline for Follow-up Observations with Optical Telescopes
