We propose an extensive investigation of the impact of stellar high-energyradiation on the planet- forming molecular stellar environments by combiningX-ray information with novel far-infrared spectroscopy from our Herschel KeyProject and complementary mid-infrared spectroscopy from Spitzer. The principalgoals are, i) to identify X-ray tracers in the Herschel spectral range, ii) tostudy the potential impact of X-rays on circumstellar material based oncorrelation studies, and iii) to model physical and chemical conditions in theregions where the X-ray impact is significant. We wish to understand how X- rayradiation influences star- and planet formation through physical and chemicalprocessing of circumstellar material. The astrobiologically important water plays a key role in this project.
A gas density drop in the inner 6 AU of the transition disk around the Herbig Ae star HD 139614 . Further evidence for a giant planet inside the disk? |Carmona, A., Thi, W. F., et al. | A&A | 598-118 | 2017 | 2017A&A...598A.118C | http://ui.adsabs.harvard.edu/#abs/2017A&A...598A.118C
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
X-ray emission from Ae/Be Herbig stars due to disc-stellar magnetosphere interaction |Ryspaeva, Elizaveta, Kholtygin, Alexander, | MNRAS | 521-2427 | 2023 | 2023MNRAS.521.2427R | http://ui.adsabs.harvard.edu/#abs/2023MNRAS.521.2427R
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
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
2011-08-09T07:33:30Z/2012-02-23T15:02:34Z
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.
European Space Agency, Prof Manuel Guedel, 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
