A dataset provided by the European Space Agency

Name: The hard X-ray emission of Class I-II YSOs and the origin of the 6.4 keV Fe line
Published: 2018-09-01T22:00:00Z

Proposal ID	080003
Title	The hard X-ray emission of Class I-II YSOs and the origin of the 6.4 keV Fe line
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800030801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800030901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800031001
DOI	https://doi.org/10.5270/esa-5a80qtq
Principal Investigator, PI	Prof Salvatore Sciortino
Abstract	ClassvirgulI and II YSOs are bright sources of soft (< 10 keV) X-rays, but verylittle is known of their hard (> 10 keV) X-ray emission and of theirinter-relation. Those YSOs can exhibit emission in the Fe Kalpha line at 6.4keV. Its origin and site of production is still controversial, e.g., being dueto flare reverberation or accelerated particles hitting the corona or thesurrounding inner part of the circumstellar disk. Time resolved spectroscopymade possible with the proposed 300 ks long joint simultaneous XMM-EPIC andNustar observations of Elias29, in the nearby (120 pc) rho Oph SFR, and of theother YSOs in the Nustar FOV will allow us to investigate, for the first time,these open questions.
Publications	Deep X-ray view of the Class I YSO Elias 29 with XMM-Newton and NuSTAR \|Pillitteri, I., Sciortino, S., et al. \| A&A \| 623-67 \| 2019 \| 2019A&A...623A..67P \| http://ui.adsabs.harvard.edu/#abs/2019A&A...623A..67P The complex phenomena of young stellar objects revealed by their X-ray variability \|Sciortino, S., Flaccomio, E., et al. \| AN \| 340-334 \| 2019 \| 2019AN....340..334S \| http://ui.adsabs.harvard.edu/#abs/2019AN....340..334S A new multiwavelength census of blazars \|Paggi, A., Bonato, M., et al. \| A&A \| 641-62 \| 2020 \| 2020A&A...641A..62P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...641A..62P 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	2017-08-13T16:17:25Z/2017-08-18T22:17:17Z
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	2018-09-01T22:00:00Z
Keywords	"kev xray emission", "exhibit emission", "hard xray emission", "xmm epic", "flare reverberation", "XMM", "circumstellar disk", "fe kalpha line", "bright sources", "nustar fov", "ii ysos", "inter relation", "kev fe line", "kev xray", "EPIC", "time resolved spectroscopy", "accelerated particles hitting"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Salvatore Sciortino, 2018, 'The hard X-ray emission of Class I-II YSOs and the origin of the 6.4 keV Fe line', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5a80qtq