'Vela pulsar' diaporamas de présentation

????????? ---- ????????? (Pulsar Astronomy: 4ed. Chap. 7)

786 views • 62 slides

AAVS 0.5: An Overview

AAVS 0.5: An Overview. Peter Hall ICRAR/Curtin, Bologna, October 22, 2012. What is AAVS 0.5?. 16-element LPDA array (70-450 MHz) located at the Murchison Radioastronomy Observatory Specifically, within the site designated for the MWA precursor Similar to one (of several) AAVS 0 arrays

197 views • 11 slides

science with 40 IceCube strings

science with 40 IceCube strings. IOFG 2010 Francis Halzen. neutrinos with 40 strings. We have measured the atmospheric neutrino spectrum to an energy of 400 TeV. The data is consistent with the predicted energy dependence. IceCube can therefore search for cosmic neutrinos

175 views • 10 slides

X-Ray Spins and Radio Speeds: Probing Pulsar Birth Kinematics with CXO and the VLBA

It is now well known that the symmetry axes of the Crab and Vela pulsar wind nebulae (red) lie rather close to their proper motion vectors (green). X-Ray Spins and Radio Speeds: Probing Pulsar Birth Kinematics with CXO and the VLBA. Is this Coincidence? Is this Physics ?

188 views • 1 slides

Abstract

Gamma-ray Large Area Space Telescope. GLAST needs contemporaneous timing measurements.

102 views • 1 slides

Gamma Ray Pulsar Candidates for GLAST

Coordinated pulsar timing campaigns for GLAST.

81 views • 1 slides

Abstract

Gamma-ray Large Area Space Telescope. GLAST needs contemporaneous timing measurements.

125 views • 1 slides