A dataset provided by the European Space Agency

Name: Characterizing the X-ray properties of the earliest magnetic stars
Published: 2014-03-23T00:00:00Z

Proposal ID	069021
Title	Characterizing the X-ray properties of the earliest magnetic stars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690210101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690210201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690210301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690210401
DOI	https://doi.org/10.5270/esa-7gbs3b9
Principal Investigator, PI	Dr Yael Naze
Abstract	The recent detection of magnetic fields in massive stars has profoundly changedour understanding of the structure and evolution of these objects. In addition,detailed modelling shows that intense magnetic fields can have a strong impacton the X-ray emission. Currently, only a few tens of magnetic hot stars areknown, not all of them have been observed at high energies. The observeddiversity of behaviours in the few studied objects actually prevent us fromrecognizing the overall trends. By extending the sample size, we will be able toundertake such a systematic study of the X-ray properties of magnetic massivestars, which will help us better understand which parameters govern theirhigh-energy emission.
Publications	X-Ray Emission from Magnetic Massive Stars \|Naze Yael Petit Veronique et al. \| ApJS \| 215-10 \| 2014 \| 2014ApJS..215...10N \| http://ui.adsabs.harvard.edu/#abs/2014ApJS..215...10N B fields in OB stars (BOB): FORS 2 spectropolarimetric follow-up of the two rare rigidly rotating magnetosphere stars HD 23478 and HD 345439 \|Hubrig S. Scholler M. et al. \| A&A \| 578-3 \| 2015 \| 2015A&A...578L...3H \| http://ui.adsabs.harvard.edu/#abs/2015A&A...578L...3H The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The detection of variable radio emission from the fast rotating magnetic hot B-star HRxA07355 and evidence for its X-ray aurorae \|Leto P. Trigilio C. et al. \| MNRAS \| 467-2820 \| 2017 \| 2017MNRAS.467.2820L \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.467.2820L Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz Tobias \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P Analysis of the X-ray emission of OB stars II: B stars \|Ryspaeva Elizaveta Kholtygin Alexander \| RAA \| 19-120 \| 2019 \| 2019RAA....19..120R \| http://ui.adsabs.harvard.edu/#abs/2019RAA....19..120R 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 Discovery of extraordinary X-ray emission from magnetospheric interaction in the unique binary stellar system u03f5 Lupi \|Das B. Petit V. et al. \| MNRAS \| 522-5805 \| 2023 \| 2023MNRAS.522.5805D \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.522.5805D Discovery of magnetospheric interactions in the doubly magnetic hot binary u03f5 Lupi \|Biswas Ayan Das Barnali et al. \| MNRAS \| 523-5155 \| 2023 \| 2023MNRAS.523.5155B \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.523.5155B 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	2012-08-10T23:04:55Z/2013-03-05T01:12:21Z
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	2014-03-23T00:00:00Z
Last Update	2025-01-27
Keywords	"sample size", "objects actually", "magnetic fields", "profoundly changed", "overall trends", "magnetic hot stars", "intense magnetic fields", "xray properties", "energy emission", "massive stars", "xray emission", "parameters govern", "magnetic massive stars", "earliest magnetic stars"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Yael Naze, 2014, 'Characterizing the X-ray properties of the earliest magnetic stars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7gbs3b9