A dataset provided by the European Space Agency

Name: Identifying the companions of chemically peculiar red giants
Published: 2017-02-15T23:00:00Z

Proposal ID	076172
Title	Identifying the companions of chemically peculiar red giants
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761720101
DOI	https://doi.org/10.5270/esa-urm6jhs
Principal Investigator, PI	Dr Gerardo Luna
Abstract	Although the peculiar surface abundances of Tc-poor S stars in six symbioticsbinaries suggest that the compact object should be a white dwarf, the X-rayspectrum from at least one member of this class points to the presence of aneutron star. For that object, the X-ray spectrum can be modeled as dueComptonized black-body emission with the seed-photons coming from the neutronstar. To determine if chemically peculiar symbiotics host a white dwarf or aneutron star, we propose to obtain XMM-Newton X-ray spectra of four suchsymbiotics. This proposal has implications for our understanding of the originof polluted atmospheres and of binary stellar evolution.
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 X-rays and TESS observations of symbiotic binary stars \|Lima, I. J., Luna, G. J. M., et al. \| BAAA \| 64-59 \| 2023 \| 2023BAAA...64...59L \| http://ui.adsabs.harvard.edu/#abs/2023BAAA...64...59L 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	2016-01-27T21:27:48Z/2016-01-28T17:11:08Z
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	2017-02-15T23:00:00Z
Keywords	"binary stellar evolution", "XMM", "xray spectrum", "symbiotics binary", "polluted atmosphere", "neutron star", "white dwarf", "red giants", "compact object", "XMM-Newton", "seed photons", "surface abundance"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gerardo Luna, 2017, 'Identifying the companions of chemically peculiar red giants', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-urm6jhs