A dataset provided by the European Space Agency

Name: X-ray emission from AGB stars
Published: 2013-09-12T00:00:00Z

Proposal ID	069380
Title	X-ray emission from AGB stars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693800101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693800301
DOI	https://doi.org/10.5270/esa-6odmbvd
Principal Investigator, PI	Dr Sofia Ramstedt
Abstract	Although the Asymptotic Giant Branch (AGB) stars are well studied in someaspects, there are several properties that remain unexplored. For instance, therole of magnetic fields for the large-scale structure and dynamics of thecircumstellar envelope (CSE) has not been established. Recent results from maserpolarimetry observations indicate strong magnetic fields throughout the innerCSE. These need to be confirmed by the detection of X-ray emission from coronalactivity. We propose to observe three low- mass-loss rate, close (<300 pc), AGBstars, in order to detect and establish the origin of X-ray emission. Theobservations would be a follow-up to our recent archival search that resulted innew X-ray detections of two AGB stars.
Publications	Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y 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 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 AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions \|Ortiz, R., Guerrero, M. A., \| ApJ \| 912-93 \| 2021 \| 2021ApJ...912...93O \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...912...93O 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	2012-06-10T07:32:42Z/2012-08-24T11:50:18Z
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	2013-09-12T00:00:00Z
Keywords	"magnetic fields", "magnetic fields throughout", "coronal activity", "x ray emission", "agb stars", "xray detections", "maser polarimetry", "archival search", "circumstellar envelope cse", "scale structure", "xray emission", "inner cse"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Sofia Ramstedt, 2013, 'X-ray emission from AGB stars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6odmbvd