A dataset provided by the European Space Agency

Name 090441
Title Searching For Evidence of Magnetospheric Interaction in Epsilon Lupi
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0904410401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0904410501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0904410601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0904410701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0904410801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0904410901

DOI https://doi.org/10.57780/esa-pupcvrm
Author European Space Agency
Description Epsilon Lupi is the only close binary star system where both massive
main-sequence components have strong magnetic fields. Thus it is a natural
laboratory for the study of the influence of magnetism on binarity. We have
discovered radio emissions from this system that revealed double-peaked
enhancement near the periastron phase, as well as pseudo-cyclic variations
across the orbital phase. The double-peak enhancement is likely to be an effect
of magnetospheric interaction. If this scenario is correct, one would also
expect X-ray counterparts to the radio enhancements in the form of enhancement
in the X-ray light curve at similar phases. Thus we request 55 ks of XMM-Newton
time to search for the evidence of magnetospheric interaction and orbital variability in our unique target.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-08-17T05:51:00Z/2022-09-08T08:38:31Z
Version 20.08_20220509_1852
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 2023-09-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, Searching For Evidence Of Magnetospheric Interaction In Epsilon Lupi, 20.08_20220509_1852, European Space Agency, https://doi.org/10.57780/esa-pupcvrm