A dataset provided by the European Space Agency

Name: X-rays from FU Orionis Stars
Published: 2008-06-22T00:00:00Z

Proposal ID	050242
Title	X-rays from FU Orionis Stars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502420101
DOI	https://doi.org/10.5270/esa-7ug68yl
Principal Investigator, PI	Dr Stephen Skinner
Abstract	FU Orionis objects (FUors) are a remarkable class of low-mass pre-main-sequencestars that undergo dramatic optical outbursts attributed to an increase of theaccretion rate onto the star. Little is known about their X-ray properties butwe have recently obtained first detections of unusual X-ray emission from theprototype FU Ori and hard X-rays from the FUor 1735 Cyg. We propose here toobserve five additional FUors with EPIC, of which two are classical FUors withhistorical outbursts (V346 Nor, Reipurt50N) and three are spectroscopic FUorswhich may be outburst precursors. These observations will double the number ofFUors observed in X-rays and provide a larger sample needed to reliablydetermine the X-ray properties of the class and identify emission mechanisms.
Publications	Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C 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 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	2007-05-23T09:44:16Z/2007-05-23T19:29:06Z
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	2008-06-22T00:00:00Z
Last Update	2025-01-27
Keywords	"larger sample", "accretion rate", "EPIC", "spectroscopic fuors", "hard xray", "classical fuors", "additional fuors", "optical outburst attributed", "fu orionis stars", "xray properties", "fuor 1735 cyg", "x rays", "xray emission", "prototype fu ori", "outburst precursors", "emission mechanisms", "historical outburst v346"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Stephen Skinner, 2008, 'X-rays from FU Orionis Stars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7ug68yl