A dataset provided by the European Space Agency

Name: X-RAY EMISSION FROM ACCRETING FU ORIONIS OBJECTS
Published: 2006-02-18T00:00:00Z

Proposal ID	020515
Title	X-RAY EMISSION FROM ACCRETING FU ORIONIS OBJECTS
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205150101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205150401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205150501
DOI	https://doi.org/10.5270/esa-6znr5vj
Principal Investigator, PI	Dr STEPHEN SKINNER
Abstract	FU Orionis objects (FUors) are a remarkable class of low-mass pre-main-sequencestars that are undergoing disk accretion at very high rates. The classical FUorshave all experienced dramatic optical outbursts attributed to a sudden increasein the disk accretion rate. Because of their youth and strong accretionsignatures, FUors should be X-ray sources. Surprisingly, X-ray data for FUorsare almost nonexistent and little is known about their X-ray attributes. Wepropose to observe three FUors with XMM-EPIC in order to determine the basicX-ray properties of the class. Our targets include the prototype FU Orionis andthe classical FUor V1057 Cyg, which is known to have been a T Tauri star priorto its optical outburst in 1970.
Publications	The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The Unusual X-Ray Spectrum of FU Orionis \|Skinner, Stephen L., Briggs, Kevin R., \| ApJ \| 643-995 \| 2006 \| 2006ApJ...643..995S \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...643..995S An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F X-ray Emission from the Pre-Main Sequence Systems FU Orionis and T Tauri \|Skinner, Stephen, Gudel, Manuel, et al. \| Ap&SS \| 304-165 \| 2006 \| 2006Ap&SS.304..165S \| http://ui.adsabs.harvard.edu/#abs/2006Ap&SS.304..165S Chandra Reveals Variable Multi-component X-ray Emission From FU Orionis \|Skinner, Stephen L., Gudel, Manuel, et al. \| ApJ \| 722-1654 \| 2010 \| 2010ApJ...722.1654S \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...722.1654S The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P An X-Ray Survey of the Young Stellar Population of the Lynds 1641 and Iota Orionis Regions \|Pillitteri, I., Wolk, S. J., et al. \| ApJ \| 768-99 \| 2013 \| 2013ApJ...768...99P \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...768...99P The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H A Comparison of the X-Ray Properties of FU Ori-type Stars to Generic Young Stellar Objects \|Kuhn, Michael A., Hillenbrand, Lynne A., \| ApJ \| 883-117 \| 2019 \| 2019ApJ...883..117K \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...883..117K Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P Chandra Resolves the Double FU Orionis System RNO 1B/1C in X-Rays \|Skinner, Stephen L., G\\u00fcdel, Manuel, \| AJ \| 159-221 \| 2020 \| 2020AJ....159..221S \| http://ui.adsabs.harvard.edu/#abs/2020AJ....159..221S An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q A chemical map of the outbursting V883 Ori system: vertical and radial structures \|Ru\\u00edz-Rodr\\u00edguez, D. A., Williams, J. P., et al. \| MNRAS \| 515-2646 \| 2022 \| 2022MNRAS.515.2646R \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515.2646R 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	2004-03-08T19:24:32Z/2004-08-25T10:03:20Z
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	2006-02-18T00:00:00Z
Keywords	"classical fuors", "xmm epic", "optical outburst", "xray sources", "xray data", "XMM", "accretion signatures", "x ray emission", "tauri star", "basic xray properties", "disk accretion", "disk accretion rate", "EPIC", "xray attributes", "optical outburst attributed", "prototype fu orionis"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr STEPHEN SKINNER, 2006, 'X-RAY EMISSION FROM ACCRETING FU ORIONIS OBJECTS', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6znr5vj