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- W2033888906 abstract "view Abstract Citations (22) References (24) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The hard X-ray spectrum of X Per. Worrall, D. M. ; Knight, F. K. ; Nolan, P. L. ; Rothschild, R. E. ; Levine, A. M. ; Primini, F. A. ; Lewin, W. H. G. Abstract Results of observations of 3U 0352 + 30, the source associated with the X Persei system, in the energy range 12-180 keV are reported. The measurements were made on 1978 August 22 with the UCSD/MIT High-Energy X-ray and Low-Energy Gamma-ray Experiment on HEAO 1. Data taken simultaneously in the energy range 2-50 keV indicate that, in addition to a 7 keV thermal bremsstrahlung component, there is a second component of higher energy. It is found that this higher energy component fits a power law of photon index 1.3 (+0.4, -0.5) and is pulsed at the 13.95 minute period of the lower energy component. Publication: The Astrophysical Journal Pub Date: July 1981 DOI: 10.1086/183583 Bibcode: 1981ApJ...247L..31W Keywords: Binary Stars; Bremsstrahlung; Neutron Stars; Stellar Luminosity; X Ray Sources; X Ray Spectra; Dwarf Stars; Giant Stars; Spectrum Analysis; Stellar Spectra; Astronomy full text sources ADS | data products SIMBAD (1)" @default.
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- W2033888906 date "1981-07-01" @default.
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- W2033888906 title "The hard X-ray spectrum of X Persei" @default.
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