| Proposal ID | 087092 |
| Title | THE HIGH ENERGY SIGNATURE OF MAGNETISM IN RHO OPH A |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0870920101 |
| DOI | https://doi.org/10.57780/esa-7x39ypu |
| Principal Investigator, PI | Dr Scott Wolk |
| Abstract | Periodically pulsed X-ray emission from the nearby B2 star Rho Oph A have beendiscovered along with a variable magnetic field and strongly modulated radioemission. All these observations fit in a model of an oblique magnetic rotator,where, alternatively, the magnetic poles and their radio emission point towardsthe Earth. In this proposal we request to use NuSTAR and XMM-Newton to monitorRho Oph A for about two rotational periods (total exposure ~140 ks) in order toclarify the link between X-rays, radio emission and magnetism which requires usto firmly characterize its high energy (> 10 keV) emission. The hard X-rayspectrum will provide a clear signature of non-thermal emission and a betterknowledge of the auroral emission and particle acceleration in magnetic B stars. |
| Publications |
|
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2020-09-13T11:46:45Z/2020-09-14T12:23:30Z |
| Version | 18.02_20200221_1200 |
| 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 | 2021-10-15T00:00:00Z |
| Keywords | "NuSTAR", "variable magnetic field", "kev emission", "XMM", "hard xray spectrum", "modulated radio emission", "magnetic poles", "auroral emission", "xmm newton", "energy signature", "radio emission", "particle acceleration", "rho oph", "XMM-Newton", "oblique magnetic rotator", "nonthermal emission" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Scott Wolk, 2021, 'THE HIGH ENERGY SIGNATURE OF MAGNETISM IN RHO OPH A', 18.02_20200221_1200, European Space Agency, https://doi.org/10.57780/esa-7x39ypu |