Proposal ID | 040212 |
Title | A survey of X-ray emission in magnetic Be stars |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402120101 |
DOI | https://doi.org/10.5270/esa-nw9ky4s |
Principal Investigator, PI | Dr Fabio Favata |
Abstract | We propose to perform a survey of the X-ray emission from Be stars, of both themagnetic and non-magnetic variety. Remarkably, only two Be stars (apart from thevery peculiar gamma Cas variety) have been observed in X-rays in recent times(beta Cep and lambda Eri), with very interesting results; no other Be star hasbeen observed in X-rays in the post-ROSAT era. The present survey is thus neededto bring the study of X-ray emission from Be stars, with the attendinginteresting physics of shocked winds (either magnetically confined or not) anddecretion disks into the modern era. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, RGS1, RGS2 |
Temporal Coverage | 2006-12-06T20:42:14Z/2007-04-29T14:56:20Z |
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 | 2009-03-12T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "shocked winds", "post rosat era", "lambda eri", "gamma cas", "ROSAT", "xray emission", "decretion dis", "stars apart", "beta cep", "magnetically confined", "modern era" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Fabio Favata, 2009, 'A survey of X-ray emission in magnetic Be stars', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-nw9ky4s |