A dataset provided by the European Space Agency

Name: X-ray Emission from Protostars SSC_20
Published: 2002-07-13T00:00:00Z

Proposal ID	011112
Title	X-ray Emission from Protostars SSC_20
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111120101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111120201
DOI	https://doi.org/10.5270/esa-0u3vani
Principal Investigator, PI	Dr Michael Watson
Abstract	GT- Observations with ROSAT and ASCA have shown that X-rays can be efficientlydetected from young objects deeply embedded in molecular clouds, extinction upto Av=40 or more, implying substantial X-ray luminosities: Lx=1E32-1E34 erg/s.X-rays are expected to strongly influence the physical state of the protostellargas and dust, with new implications for the early solar system. We propose toobtain 1-10 keV spectra of two evolved protostars already known in X-rays, inorder to accurately measure the plasma temperature and the extinction; we willalso attempt to detect for the first time a very young protostar, still embeddedin a thick circumstellar envelope.
Publications	Radio and X-ray variability of young stellar objects in the Coronet cluster \|Forbrich J. Preibisch Th. \| A&A \| 446-155 \| 2006 \| 2006A&A...446..155F \| http://ui.adsabs.harvard.edu/#abs/2006A&A...446..155F 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 Determination of the gas-to-dust ratio in nearby dense clouds using X-ray absorption measurements \|Vuong M. H. Montmerle T. et al. \| A&A \| 408-581 \| 2003 \| 2003A&A...408..581V \| http://ui.adsabs.harvard.edu/#abs/2003A&A...408..581V X-ray detections of two young bona-fide brown dwarfs \|Bouy H. \| A&A \| 424-619 \| 2004 \| 2004A&A...424..619B \| http://ui.adsabs.harvard.edu/#abs/2004A&A...424..619B The X-ray emission from Young Stellar Objects in the rho Ophiuchi cloud core as seen by XMM-Newton. \|Ozawa H. Grosso N. \| A&A \| 429-963 \| 2005 \| 2005A&A...429..963O \| http://ui.adsabs.harvard.edu/#abs/2005A&A...429..963O A survey for Fe 6.4 keV emission in young stellar objects in rho Oph: The strong fluorescence from Elias 29 \|Favata F. Micela G. et al. \| A&A \| 433-1047 \| 2005 \| 2005A&A...433.1047F \| http://ui.adsabs.harvard.edu/#abs/2005A&A...433.1047F The X-ray emission from Young Stellar Objects in the rho Ophiuchi cloud core as seen by XMM-Newton \|Ozawa H. Grosso N. \| A&A \| 438-661 \| 2005 \| 2005A&A...438..661O \| http://ui.adsabs.harvard.edu/#abs/2005A&A...438..661O XMM-Newton data processing for faint diffuse emission. Proton flares exposure maps and report on EPIC MOS1 bright CCDs contamination \|Pradas J. Kerp J. \| A&A \| 443-721 \| 2005 \| 2005A&A...443..721P \| http://ui.adsabs.harvard.edu/#abs/2005A&A...443..721P The XMM-Newton EPIC background and the production of background blank sky event files \|Carter J. A. Read A. M. \| A&A \| 464-1155 \| 2007 \| 2007A&A...464.1155C \| http://ui.adsabs.harvard.edu/#abs/2007A&A...464.1155C XMM-Newton local bubble and galactic halo survey \|Freyberg M. J. Breitschwerdt D. \| AN \| 324-162 \| 2003 \| 2003AN....324..162F \| http://ui.adsabs.harvard.edu/#abs/2003AN....324..162F X-rays from the Local Bubble \|Freyberg Michael J. \| Ap&SS \| 289-229 \| 2004 \| 2004Ap&SS.289..229F \| http://ui.adsabs.harvard.edu/#abs/2004Ap&SS.289..229F 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 Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog \|Georgakakis A. E. Chavushyan V. et al. \| MNRAS \| 367-1017 \| 2006 \| 2006MNRAS.367.1017G \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367.1017G 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 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 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 A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi J. A. Albacete Colombo J. F. et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C The XMM-Newton serendipitous source catalogue \|Watson M. G. Pye J. P. et al. \| AN \| 324-89 \| 2003 \| 2003AN....324...89W \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...89W The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca A. Molendi S. \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D Automatic Classification of Time-variable X-Ray Sources \|Lo Kitty K. Farrell Sean et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L 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-Zeldovich 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 A survey of stellar X-ray flares from the XMM-Newton serendipitous source catalogue: HIPPARCOS-Tycho cool stars \|Pye J. P. Rosen S. et al. \| A&A \| 581-28 \| 2015 \| 2015A&A...581A..28P \| http://ui.adsabs.harvard.edu/#abs/2015A&A...581A..28P Results from DROXO. IV. EXTraS discovery of an X-ray flare from the Class I protostar candidate ISO-Oph 85 \|Pizzocaro D. Stelzer B. et al. \| A&A \| 587-36 \| 2016 \| 2016A&A...587A..36P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...587A..36P 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 High-energy processes in low-mass protostars - an X-ray to radio multi-wavelength perspective \|Forbrich Jan \| PhDT \| 0-5 \| 2007 \| 2007PhDT.........5F \| http://ui.adsabs.harvard.edu/#abs/2007PhDT.........5F 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 The Spectrum of the Universe \|Hill Ryley Masui Kiyoshi W. \| ApSpe \| 72-663 \| 2018 \| 2018ApSpe..72..663H \| http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H 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 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 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 A Statistical Study of Soft X-Ray Flares on Solar-type Stars \|Zhao Z. H. Hua Z. Q. et al. \| ApJ \| 961-130 \| 2024 \| 2024ApJ...961..130Z \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..130Z 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	2001-02-19T21:13:11Z/2001-04-09T16:04:59Z
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	2002-07-13T00:00:00Z
Last Update	2025-01-27
Keywords	"thick circumstellar envelope", "protostars ssc_20", "1e32 1e34 erg", "evolved protostars", "kev spectra", "ROSAT", "objects deeply embedded", "x ray emission", "solar system", "protostellar gas", "plasma temperature", "molecular clouds"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Michael Watson, 2002, 'X-ray Emission from Protostars SSC_20', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0u3vani