A dataset provided by the European Space Agency

Proposal ID 0920009
Obs ID 09200090001, 09200090002, 09200090003
Title Hercules X-1: Variability of the cyclotron line energy Ecyc and the question of NS free precession
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:0920009
DOI https://doi.org/10.57780/esa-cmsyik8
Author Staubert
Abstract We propose to observe Her X-1 during INTEGRAL s AO-9 for a total observing time of 600 ksec: covering one Main-On with two INTEGRAL orbits, the first near the maximum of the Main-On , the second during its decay, plus one INTEGRAL orbit during the following Short-On . Our general objective is to continue the long-term covering of this enigmatic source by INTEGRAL, in order to investigate two (intimately related) aspects: A. the physics of generating the cyclotron line and the reasons behind the variability of Ecyc as a function of time, luminosity, 35 day precession-phase and 1.24 s pulse-phase, and B. the question whether the neutron star (NS) does really precess with a period of 35 days in strict synchronization with the accretion disk. If the observed systematic variations of the shape of the pulse profiles are indeed due to the NS s precession, then we would have to conclude that the precessional period is changing by a few percent every few years, which most likely requires some changes in the structure of matter and/or magnetic field of the NS s interior. This may open a new channel to the understanding of the properties of matter at supra-nuclear densities. On the other hand, some observational results seriously challenge the idea of NS precession in Her X-1.
Publications
Temporal Coverage 2012-04-01T06:11:44Z / 2012-04-21T21:11:21Z
Version 1.0
Mission Description The INTEGRAL (International Gamma-Ray Astrophysics Laboratory) mission, launched by the European Space Agency (ESA) on October 17, 2002, was designed to study high-energy phenomena in the universe. INTEGRAL was operating until february 2025 and it was equipped with three high-energy instruments: the Imager on Board the INTEGRAL Satellite (IBIS), the Spectrometer on INTEGRAL (SPI), and the JEM-X (Joint European Monitor for X-rays). Its Optical Monitoring Camera (OMC) provided optical V-band magnitude measurements, complementing the high-energy observations.
Creator Contact https://www.cosmos.esa.int/web/integral/helpdesk
Date Published 2025-03-25T09:54:36Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Staubert, 2025, 'Hercules X-1: Variability of the cyclotron line energy Ecyc and the question of NS free precession', 1.0, European Space Agency, https://doi.org/10.57780/esa-cmsyik8