Observations of Millisecond Pulsars with the Fermi Large Area Telescope

Details Observations of Millisecond Pulsars with the Fermi Large Area Telescope Observations of Millisecond Pulsars with the Fermi Large Area Telescope

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.1602k&link_type=abstract

American Astronomical Society, HEAD meeting #11, #16.02; Bulletin of the American Astronomical Society, Vol. 41, p.679

Astronomy and Astrophysics

Astronomy

Scientific paper

Millisecond pulsars (MSPs) have been firmly established as a class of high-energy, >0.1 GeV, emitters via the detection of pulsations, using radio timing solutions, of at least nine MSPs with the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope. The LAT data suggest that the emission mechanisms in gamma-ray MSPs are the same as those powering younger gamma-ray pulsars. We will present the MSP results from the LAT including the implications from the LAT detection of gamma-ray emission from the globular cluster 47 Tucanae, which hosts at least twenty-three radio-loud MSPs.

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