activity
20002011
most citedMagnetars as cooling neutron stars with internal heating

66 citations · 243 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2011★ 40 cited

Soft and Hard X-Ray Emissions from the Anomalous X-ray Pulsar 4U 0142+61 Observed with Suzaku

Teruaki Enoto, Kazuo Makishima, Kazuhiro Nakazawa +4

The anomalous X-ray pulsar 4U 0142+61 was observed with Suzaku on 2007 August 15 for a net exposure of -100 ks, and was detected in a 0.4 to ~70 keV energy band. The intrinsic puls…

astro-ph.HE2010★ 11 cited

Suzaku Observation of the Anomalous X-ray Pulsar 1E 1841-045

Mikio Morii, Shunji Kitamoto, Noriaki Shibazaki +7

We report the results of a Suzaku observation of the anomalous X-ray pulsar (AXP) 1E 1841-045 at a center of the supernova remnant Kes 73. We confirmed that the energy-dependent sp…

astro-ph2008★ 5 cited

Search for Near-Infrared Pulsation of the Anomalous X-ray Pulsar 4U 0142+61

Mikio Morii, Naoto Kobayashi, Nobuyuki Kawai +4

We have searched for pulsation of the anomalous X-ray pulsar (AXP) 4U 0142+61 in the K' band ( m) using the fast-readout mode of IRCS at the Subaru 8.2-m tel…

astro-ph2007★ 2 cited

Suzaku Observation of AXP 1E 1841-045 in SNR Kes 73

M. Morii, S. Kitamoto, N. Shibazaki +7

Anomalous X-ray pulsars (AXPs) are thought to be magnetars, which are neutron stars with ultra strong magnetic field of -- G. Their energy spectra below 10…

astro-ph2007★ 22 cited

Uniting the Quiescent Emission and Burst Spectra of Magnetar Candidates

Yujin E. Nakagawa, Atsumasa Yoshida, Kazutaka Yamaoka +1

Spectral studies of quiescent emission and bursts of magnetar candidates using XMM-Newton, Chandra and Swift data are presented. Spectra of both the quiescent emission and the burs…

astro-ph2006★ 66 cited

Magnetars as cooling neutron stars with internal heating

A. D. Kaminker, D. G. Yakovlev, A. Y. Potekhin +3

We study thermal structure and evolution of magnetars as cooling neutron stars with a phenomenological heat source in a spherical internal layer. We explore the location of this la…