A dataset provided by the European Space Agency

Proposal ID 0940023
Obs ID 09400230006, 09400230007, 09400230008, 09400230009, 09400230010, 09400230011, 09400230012, 09400230013
Title Following the evolution of the X-ray emitting structure with luminosity in transient accreting pulsars.
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:0940023
DOI https://doi.org/10.57780/esa-aocium5
Author Klochkov
Abstract We propose a Target of Opportunity Observation whenever one of the transient accreting pulsars from the provided list of sources enters an outburst. The main scientific goal of the proposal is to identify and study different accretion regimes that might be at work in the observed source depending on the luminosity level - a new very promising approach to understand the physics inside the emitting accretion column/mound on the neutron star. Different accretion regimes lead to different luminosity-dependencies of the broad-band spectral continuum and the cyclotron feature. We demonstrate that the observed slopes of the dependencies at different luminosities can quantitatively be compared with theoretical predictions. We will also search for transitions from one accretion regime to another that so far have not been seen in any source, but, if observed, would provide an ultimate test for the theory of the X-ray emitting structure on accreting pulsars. The proposal is focused on those X-ray pulsars the spectra of which contain an evidence or an indication of a cyclotron scattering feature but for which the evolution of the broad-band X-ray spectrum with luminosity (i.e. throughout an outburst) has not been so far studied in details. We request a total of 800 ksec of exposure time divided into several pointings to follow the spectral evolution with flux of the source entered in outburst.
Publications
Temporal Coverage 2012-01-17T11:38:31Z / 2012-02-08T11:13:01Z
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 2025-03-25T09:54:37Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Klochkov, 2025, 'Following the evolution of the X-ray emitting structure with luminosity in transient accreting pulsars.', 1.0, European Space Agency, https://doi.org/10.57780/esa-aocium5