A dataset provided by the European Space Agency

Name 055012
Title Is NeII a Tracer for X-Rays in Disks around Tauri Stars?
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550120701

DOI 10.5270/esa-wkzgw12
Author Dr Manuel Guedel
Description Although dust grains dominate the appearance of protoplanetary disks because of their high opacity, the key processes for disk evolution and planetesimal formation are driven through the dynamical state of the gas. In contrast to the dust component, we do not have a similar knowledge of the gas component. One of the Spitzer breakthroughs was the detection of the [Ne II] 12.8um line. Glassgold et al. (2007) proposed that this line provides diagnostics for a warm disk surface layer that is heated and ionized by stellar X-rays. A correlation of the [Ne II] luminosity with the X-ray luminosity is expected. The statistical sample so far available is insufficient to test this hypothesis. We aim at significantly enlarging the sample, with the goal of confirming or refuting this model.
Publication On the origin of [NeII] 12.81 mum emission from pre-main sequence stars: Disks, jets, and accretion . Gudel, M., Lahuis, F., et all. . A&A . 519-113 . 2010 . 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 all. . ApJ . 747-23 . 2012 . 2012ApJ...747L..23K ,
Estimation of the XUV radiation onto close planets and their evaporation . Sanz-Forcada, J., Micela, G., et all. . A&A . 532-6 . 2011 . 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 ,
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 ,
Transitional Disks and Their Origins: An Infrared Spectroscopic Survey of Orion A . Kim, K. H., Watson, Dan M., et all. . ApJ . 769-149 . 2013 . 2013ApJ...769..149K ,
Molecules in the transition disk orbiting T Chamaeleontis . Sacco, G. G., Kastner, J. H., et all. . A&A . 561-42 . 2014 . 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 . ...,
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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 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 ,
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 ,
Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks . Dionatos, O., Woitke, P., et all. . A&A . 625-66 . 2019 . 2019A&A...625A..66D ,
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-04-02T00:00:00Z, 055012, 17.56_20190403_1200. https://doi.org/10.5270/esa-wkzgw12