A dataset provided by the European Space Agency

Name 030049
Title The X-ray emission mechanism in magnetic Be stars
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300490201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300490301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300490401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300490501

DOI https://doi.org/10.5270/esa-x7o79tw
Author Dr Fabio Favata
Description We propose to obtain RGS spectra and EPIC light curves and spectra of the
magnetic Be star beta Cep, to provide stringent tests of the magnetically
confined wind shock model proposed to explain the X-ray emission observed from
this star. Measurement of the density from the O VII triplet (as well as of the
Ne and Mg triplets), of the line broadening, and determination of the rotational
modulation of the spectral characteristics will allow to discriminate X-ray
emission due to this novel mechanism from either coronal emission or emission
due to the shocked winds observed in non-magnetic high-mass stars.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-07-27T04:06:32Z/2005-08-06T18:04:53Z
Version 17.56_20190403_1200
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 2006-11-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Fabio Favata, 2006, 030049, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-x7o79tw