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Binary Millisecond Pulsar Discovery via Gamma-Ray Pulsations
H. J. Pletsch, L. Guillemot, H. Fehrmann +150
Millisecond pulsars, old neutron stars spun-up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "…
Fermi-LAT and WMAP observations of the Puppis A Supernova Remnant
J. W. Hewitt, M. -H. Grondin, M. Lemoine-Goumard +3
We report the detection of GeV γ-ray emission from the supernova remnant Puppis A with the Fermi Gamma-Ray Space Telescope. Puppis A is among the faintest supernova remnants yet de…
Constraints on cosmic-ray efficiency in the supernova remnant RCW 86 using multi-wavelength observations
M. Lemoine-Goumard, M. Renaud, J. Vink +4
Several young supernova remnants (SNRs) have recently been detected in the high-energy and very-high-energy gamma-ray domains. As exemplified by RX J1713.7-3946, the nature of this…
Fermi LAT study of cosmic-rays and the interstellar medium in nearby molecular clouds
LAT collaboration
We report an analysis of the interstellar gamma-ray emission from the Chamaeleon, R Coronae Australis (R CrA), and Cepheus and Polaris flare regions with the Fermi Large Area Teles…
Search for Spatially Extended Fermi-LAT Sources Using Two Years of Data
Joshua Lande, Markus Ackermann, Alice Allafort +10
Spatial extension is an important characteristic for correctly associating gamma-ray-emitting sources with their counterparts at other wavelengths and for obtaining an unbiased mod…
Fermi-LAT constraints on the Pulsar Wind Nebula nature of HESS J1857+026
R. Rousseau, M. -H. Grondin, A. Van Etten +13
Since its launch, the Fermi satellite has firmly identified 5 pulsar wind nebulae plus a large number of candidates, all powered by young and energetic pulsars. HESS J1857+026 is a…