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High-energy gamma-ray emission properties of an anomalous x-ray pulsar, 4U 0142+61

Şaşmaz Muş, Sinem and Göğüş, Ersin High-energy gamma-ray emission properties of an anomalous x-ray pulsar, 4U 0142+61. In: 2011 Fermi Symposium, (Submitted)

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Abstract

Anomalous X-ray Pulsars (AXPs) are bright X-ray sources. Few AXPs emit highly pulsed emission in hard X-rays. Using data collected with the Large Area Telescope on board Fermi Gamma-ray Space Telescope, we explored high-energy gamma-ray emission from the brightest AXP, 4U 0142+61. We do not detect any significant emission from the source. Here, we present the upper limits to the persistent and pulsed emission of 4U 0142+61 in the high-energy gamma-ray domain.

Item Type:Papers in Conference Proceedings
Subjects:Q Science > QB Astronomy > QB460-466 Astrophysics
Q Science > QC Physics
ID Code:17386
Deposited By:Ersin Göğüş
Deposited On:15 Nov 2011 16:26
Last Modified:15 Nov 2011 16:26

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