A dataset provided by the European Space Agency

Name: The X-ray emission of magnetic ApBp stars
Published: 2017-04-29T22:00:00Z

Proposal ID	076039
Title	The X-ray emission of magnetic ApBp stars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760390101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760390201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760390301
DOI	https://doi.org/10.5270/esa-yafcg1u
Principal Investigator, PI	Dr Jan Robrade
Abstract	We propose XMM observations of a sample of magnetic chemically peculiar stars(Ap/Bp stars) to test them for intrinsic X-ray emission and its relation to themagnetically channelled wind shock (MCWS) model. The aim is to investigate theX-ray generating mechanisms in intermediate mass stars in greater detail.
Publications	Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2015-12-19T14:44:22Z/2016-03-20T03:52:39Z
Version	17.56_20190403_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	2017-04-29T22:00:00Z
Keywords	"bp stars", "magnetic chemically", "magnetic apbp stars", "stars ap", "xray generating mechanisms", "XMM", "xray emission", "intermediate mass stars"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jan Robrade, 2017, 'The X-ray emission of magnetic ApBp stars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-yafcg1u