Proposal ID | 002394 |
Title | Temporal-Spectral Analysis of BHC LMC X-1, LMC X-3 |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0023940101 |
DOI | https://doi.org/10.5270/esa-0w7xsub |
Principal Investigator, PI | Dr Demosthenes Kazanas |
Abstract | We propose XMM EPIC CCD observations in timing mode of theBlack Hole Candidates (BHC) LMC X-1 and LMC X-3. Our goal is to probe the spatial structure of the X-ray emittinghot coronae by the combined temporal-spectral analysis of time lags between different energy bands in the XMM range as a function of the Fourier frequency. These lags appear to be at odds with predictions of accretion disk models. The unique properties of XMM allow the search for a transition in the lag sign from positive to negative at E < 2keV, thus identifying the source of soft photons, whose Comptonization gives rise to the observed X-ray spectra and timing properties in these objests. This study will thus complement those carried out by RXTE at exclusively high (> 2 keV) X-ray energies. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2002-04-21T14:29:13Z/2002-09-26T16:43:47Z |
Version | PPS_NOT_AVAILABLE |
Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis. |
Creator Contact | https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk |
Date Published | 2005-01-01T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "bhc lmc x", "soft photons", "energy bands", "lmc x", "EPIC", "xmm epic ccd", "kev xray energies", "spatial structure", "lag sign", "time lags", "fourier frequency", "XMM", "temporal spectral analysis", "xmm range", "xray spectra", "accretion disk models" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Demosthenes Kazanas, 2005, 'Temporal-Spectral Analysis of BHC LMC X-1, LMC X-3', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-0w7xsub |