A dataset provided by the European Space Agency

Name: Characterizing the X-ray properties of the earliest magnetic stars
Published: 2011-11-05T00:00:00Z

Proposal ID	065032
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=0650320101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650320201
DOI	https://doi.org/10.5270/esa-ejw2ejo
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, and much fewer have been observed at high energies. The observeddiversity of behaviours and the small sample size actually prevent us fromrecognizing the overall trends. By doubling the sample size with a smallinvestment of time, we will be able to undertake such a systematic study of theX-ray properties of magnetic massive stars, which will help us better understandwhich parameters govern their high-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 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 On the Absence of Non-thermal X-Ray Emission around Runaway O Stars \|Toala J. A. Oskinova L. M. \| ApJ \| 838-19 \| 2017 \| 2017ApJ...838L..19T \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...838L..19T Is the Pollocks paradigm of X-ray emission for O stars correct? \|Ryspaeva E. B. Kholtygin A. F. \| AN \| 338-959 \| 2017 \| 2017AN....338..959R \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..959R Analysis of the X-ray emission of OB stars: O stars \|Ryspaeva Elizaveta Kholtygin Alexander \| RAA \| 18-104 \| 2018 \| 2018RAA....18..104R \| http://ui.adsabs.harvard.edu/#abs/2018RAA....18..104R 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 A census of young stellar population associated with the Herbig Be star HD 200775 \|Saha Piyali Gopinathan Maheswar et al. \| MNRAS \| 494-5851 \| 2020 \| 2020MNRAS.494.5851S \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.5851S 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 X-ray emission from Ae/Be Herbig stars due to disc-stellar magnetosphere interaction \|Ryspaeva Elizaveta Kholtygin Alexander \| MNRAS \| 521-2427 \| 2023 \| 2023MNRAS.521.2427R \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.521.2427R 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	2010-08-30T00:31:18Z/2010-10-16T10:41:38Z
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	2011-11-05T00:00:00Z
Last Update	2025-01-27
Keywords	"sample size", "magnetic fields", "profoundly changed", "overall trends", "magnetic hot stars", "intense magnetic fields", "xray properties", "energy emission", "massive stars", "xray emission", "sample size actually", "parameters govern", "magnetic massive stars", "earliest magnetic stars"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Yael Naze, 2011, 'Characterizing the X-ray properties of the earliest magnetic stars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ejw2ejo