Hostname: page-component-848d4c4894-8kt4b Total loading time: 0 Render date: 2024-06-22T20:31:43.900Z Has data issue: false hasContentIssue false

Herculis X1: Results and Interpretation

Published online by Cambridge University Press:  04 August 2017

Ph. Durouchoux*
Affiliation:
Service d'Astrophysique, DPhG/Ap, CEN Saclay 91191 Gif/s/Yvette, FRANCE

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The hard X-ray spectrum of Her X1 was measured for the first time with a high-resolution (1.4 keV FWHM) germanium spectrometer (LEGS: GSFC/Saclay collaboration). The observation was performed near the peak of the 0B state in the 35 day cycle and 1.24 s pulsations were observed between the energies of 20 keV and 70 keV. The best fit energies are 35 keV for an absorption line and 39 keV for an emission line. These are significantly lower energies than those derived from previous experiments.

Type
II. Accretion Powered Pulsars
Copyright
Copyright © Reidel 1987