POSSIBLE DETECTION OF AN EMISSION CYCLOTRON RESONANCE SCATTERING FEATURE FROM THE ACCRETION-POWERED PULSAR 4U 1626-67

Record Type
Journal Articles
Full Title
POSSIBLE DETECTION OF AN EMISSION CYCLOTRON RESONANCE SCATTERING FEATURE FROM THE ACCRETION-POWERED PULSAR 4U 1626-67
Author(s)
Iwakiri W, Terada Y, Mihara T, Angelini L, Tashiro M, Enoto T, Yamada S, Makishima K, Nakajima M, Yoshida A
Publication Title
ASTROPHYSICAL JOURNAL
Publication Title (abbreviated)
ASTROPHYS J
Publication Date
2012 May 20
DOI
10.1088/0004-637X/751/1/35
ISSN
0004-637X
Volume
751
Issue
1
Page Count
11
Article Number
35
Keyword(s)
Astronomy & Astrophysics, pulsars: individual (4U 1626-67), stars: magnetic field, X-rays: binaries, X-rays: stars, X-RAY PULSAR, STRONGLY MAGNETIZED PLASMA, TORQUE REVERSAL, LINE EMISSION, 4U-1626-67, FIELDS, SUZAKU, SPECTROSCOPY, HERCULES-X-1, SPECTRUM
Citation
Iwakiri W, Terada Y, Mihara T, Angelini L, Tashiro M, Enoto T, Yamada S, Makishima K, Nakajima M, Yoshida A. POSSIBLE DETECTION OF AN EMISSION CYCLOTRON RESONANCE SCATTERING FEATURE FROM THE ACCRETION-POWERED PULSAR 4U 1626-67. ASTROPHYS J. 2012;751 (1):11.
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