A dataset provided by the European Space Agency

Name: Is NeII a Tracer for X-Rays in Disks around Tauri StarsquestionMark
Published: 2010-04-02T00:00:00Z

Proposal ID	055012
Title	Is NeII a Tracer for X-Rays in Disks around Tauri Stars?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120701
DOI	https://doi.org/10.5270/esa-wkzgw12
Principal Investigator, PI	Dr Manuel Guedel
Abstract	Although dust grains dominate the appearance of protoplanetary disks because oftheir high opacity, the key processes for disk evolution and planetesimalformation are driven through the dynamical state of the gas. In contrast to thedust component, we do not have a similar knowledge of the gas component. One ofthe Spitzer breakthroughs was the detection of the Ne II 12.8um line.Glassgold et al. (2007) proposed that this line provides diagnostics for a warmdisk surface layer that is heated and ionized by stellar X-rays. A correlationof the Ne II luminosity with the X-ray luminosity is expected. The statisticalsample so far available is insufficient to test this hypothesis. We aim atsignificantly enlarging the sample, with the goal of confirming or refuting this model.
Publications	On the origin of NeII 12.81 mum emission from pre-main sequence stars: Disks, jets, and accretion \|Gudel, M., Lahuis, F., et al. \| A&A \| 519-113 \| 2010 \| 2010A&A...519A.113G \| http://ui.adsabs.harvard.edu/#abs/2010A&A...519A.113G 2M1155-79 (= T Chamaeleontis B): A Low-mass, Wide-separation Companion to the nearby, Old T Tauri Star T Chamaeleontis \|Kastner, Joel H., Thompson, Emily A., et al. \| ApJ \| 747-23 \| 2012 \| 2012ApJ...747L..23K \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...747L..23K Estimation of the XUV radiation onto close planets and their evaporation \|Sanz-Forcada, J., Micela, G., et al. \| A&A \| 532-6 \| 2011 \| 2011A&A...532A...6S \| http://ui.adsabs.harvard.edu/#abs/2011A&A...532A...6S 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 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 Transitional Disks and Their Origins: An Infrared Spectroscopic Survey of Orion A \|Kim, K. H., Watson, Dan M., et al. \| ApJ \| 769-149 \| 2013 \| 2013ApJ...769..149K \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...769..149K Molecules in the transition disk orbiting T Chamaeleontis \|Sacco, G. G., Kastner, J. H., et al. \| A&A \| 561-42 \| 2014 \| 2014A&A...561A..42S \| http://ui.adsabs.harvard.edu/#abs/2014A&A...561A..42S 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 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 High energy irradiated protoplanetary disks : the X-rays and FUV role in thermo-chemical modeling \|Aresu, Giambattista, \| PhDT \| 0-81 \| 2012 \| 2012PhDT........81A \| http://ui.adsabs.harvard.edu/#abs/2012PhDT........81A Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz, Tobias, \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks \|Dionatos, O., Woitke, P., et al. \| A&A \| 625-66 \| 2019 \| 2019A&A...625A..66D \| http://ui.adsabs.harvard.edu/#abs/2019A&A...625A..66D 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 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	2008-06-08T05:14:24Z/2009-03-16T18:40:17Z
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	2010-04-02T00:00:00Z
Keywords	"tauri stars ?.", "planetesimal formation", "statistical sample", "xray luminosity", "dust component", "key processes", "8um line", "dust grains dominate", "protoplanetary dis", "spitzer breakthroughs", "disk evolution", "ne ii", "stellar xray", "gas component"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Manuel Guedel, 2010, 'Is NeII a Tracer for X-Rays in Disks around Tauri StarsquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-wkzgw12