A dataset provided by the European Space Agency

Name 086544
Title Investigating the vertical structure of the accretion disc wind in Hercules X-1
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0865440101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0865440401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0865440501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0865440601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0865440701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0865440801

DOI https://doi.org/10.57780/esa-raxmflz
Author Mr Peter Kosec
Description Accretion disc winds in X-ray binaries are not spherically symmetric structures, but their solid angle is difficult to determine because we usually only sample specific lines of sight. We can overcome this problem by studying Hercules X-1, a binary with a precessing warped disc. Its disc wind is strongly varying within a precession cycle, indicating a small wind launching angle and strong vertical stratification. However, the available data originate from many precession cycles and could be plagued by long-term variability effects. With this proposal, we aim to finely sample the wind vertical structure within a single precession cycle, free of any long term deviations, to understand the wind launching angle, launching mechanism and to measure accurately the mass outflow rate.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2020-08-10T14:02:34Z/2020-08-16T04:41:24Z
Version 19.17_20220121_1250
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2021-08-30T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2021, 086544, 19.17_20220121_1250. https://doi.org/10.57780/esa-raxmflz