A dataset provided by the European Space Agency

Name 067354
Title X-Rays, Dust, Ice, and Gas in Time (X-DIGIT)
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673540201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673540301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673540401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673540501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673540601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673540701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673540801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673540901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673541001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673541101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673541201
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673541301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673541401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673541501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673541601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673541701

DOI https://doi.org/10.5270/esa-a2b1upz
Author European Space Agency
Description We propose an extensive investigation of the impact of stellar high-energy
radiation on the planet- forming molecular stellar environments by combining
X-ray information with novel far-infrared spectroscopy from our Herschel 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 material based on
correlation studies, 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 circumstellar material. The astrobiologically important water plays a key role in this project.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-08-09T07:33:30Z/2012-02-23T15:02:34Z
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 2013-03-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, X-Rays Comma Dust Comma Ice Comma And Gas In Time Openparx-Digitclosepar, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-a2b1upz