A dataset provided by the European Space Agency

Name 060273
Title X-Rays, Dust, Ice, and Gas in Time (X-DIGIT)
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602730101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602730701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602730901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602731101

DOI 10.5270/esa-t2edvq3
Author Dr Manuel Guedel
Description We propose an extensive investigation of the impact of stellar X-rays on the planet-forming molecular environments of T Tauri stars by combining X-ray data from XMM-Newton with novel far-infrared spectroscopy from our Herschel "Open Time Key Project" and complementary mid-infrared spectroscopy from Spitzer. The principal goals are, i) to identify X-ray tracers in the Herschel spectral range, ii) to study the potential impact of X-rays on circumstellar disks, and iii) to model physical and chemical conditions in the regions where the X-ray impact is significant. We wish to understand how X-ray radiation influences star- and planet formation through physical and chemical processing of disks. Understanding the distribution of the astrobiologically important water plays a key role.
Publication 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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
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 2009-08-24T20:33:10Z/2010-02-20T13:33:57Z
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 2011-03-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-03-23T00:00:00Z, 060273, 17.56_20190403_1200. https://doi.org/10.5270/esa-t2edvq3