Figure 4 from Possible Detection of an Emission Cyclotron Resonance Scattering Feature from the Accretion-powered Pulsar 4U 1626

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Possible Detection of an Emission Cyclotron Resonance Scattering Feature from the Accretion-powered Pulsar 4U 1626–67

Authors: W. B. Iwakiri, Y. Terada, T. Mihara, L. Angelini, M. S. Tashiro, T. Enoto, S. Yamada, K. Makishima, M. Nakajima, and A. Yoshida

Iwakiri et al. 2012 The Astrophysical Journal 751 35.

Provider: AAS Journals

Caption: Figure 4.

Energy-resolved and background-inclusive pulse profiles of 4U 1626−67. Data were folded at P _{(
Suzaku)} = 7.67795 s. Phase 0 corresponds to MJD 53803.000092755. The average background count rates of 3.5–10.0 keV, 10.0–30.0 keV, and 30.0–50.0 keV energy bands are 0.016 counts s ⁻¹, 0.49 counts s ⁻¹, and 0.086 counts s ⁻¹, respectively.

Other Images in This Article

Copyright and Terms & Conditions