Nature12917
A Millisecond Pulsar in a Stellar Triple System
Radio and Gamma-Ray Beams from Pulsars R. N. Manchester CSIRO Astronomy and Space Science Australia Telescope National Facility, Sydney Summary Pulse profiles.
Slide 1 Calculate the net force acting on a particle Mass transfer in a binary system.
RESONANT COMPTON SCATTERING AND CONNECTION BETWEEN GAMMA EMISSION AND RADIO EMISSION IN MILLISECOND PULSARS A.B. Flanchik Institute of Radio Astronomy.
LOFAR for Pulsars Ben Stappers JBCA, Manchester. Outline: LOFAR: briefly what we need from LOFAR Pros and cons of low-frequency observations How.
Zhen Yan, Zhi-Qiang Shen, Xin-Ji Wu On behalf of the Shanghai 65m Radio Telescope Team.
Pulsar Searching and Timing R. N. Manchester CSIRO Astronomy and Space Science Sydney Australia Summary Introduction to pulsars and timing Binary pulsar.
1. White Dwarf If initial star mass < 8 M Sun or so. (and remember: Maximum WD mass is 1.4 M Sun, radius is about that of the Earth) 2. Neutron Star If.
Anisotropy and Energy Spectrum of the CGB as probes of Dark Matter and Astrophysical Sources June 21-26, 2010, CCAPP, Ohio State University Shin’ichiro.
Fundamental Physics and Astrophysics using Pulsars and the SKA Jim Cordes Cornell U. Vicky Kaspi McGill U. Michael Kramer Jodrell Bank.
16 Aug 2005Jim Cordes: SKA: Introduction and Current Developments The Square Kilometer Array: Introduction and Current Developments Jim Cordes, Cornell.
