X-Rays, Dust, Ice, and Gas in Time (X-DIGIT)

Details X-Rays, Dust, Ice, and Gas in Time (X-DIGIT) X-Rays, Dust, Ice, and Gas in Time (X-DIGIT)

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop..147g&link_type=abstract

XMM-Newton Proposal ID #06735414

Mathematics

Logic

Stars, White Dwarfs, Solar System, Hd 35187, Hd 36112, Hd 50138, Hd 98922, Hd 142527, Hd 179218, Hd 139614, Hd 142666, Hd 203024, Iras 03301+3111, Iras 12496-7650, Irs 63, L1014, B1-A

Scientific paper

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.

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