Search Results - "Raassen, A J J"
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Solar chemical composition in the hot gas of cool-core ellipticals, groups, and clusters of galaxies
Published in Monthly notices of the Royal Astronomical Society. Letters (11-10-2018)“…Abstract The hot intracluster medium (ICM) pervading galaxy clusters and groups is rich in metals, which were synthesized by billions of supernovae and have…”
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Mass-invariance of the iron enrichment in the hot haloes of massive ellipticals, groups, and clusters of galaxies
Published in Monthly notices of the Royal Astronomical Society. Letters (01-07-2018)“…ABSTRACT X-ray measurements find systematically lower Fe abundances in the X-ray emitting haloes pervading groups (kT ≲ 1.7 keV) than in clusters of galaxies…”
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3
Branching Fractions and Transition Probabilities for UV Transitions in the Spectrum of Cr ii
Published in The Astrophysical journal (01-12-2023)“…Abstract We present transition probabilities for 268 spectral lines of singly ionized chromium (Cr ii ) in the wavelength region 208–414 nm. Branching…”
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First Light Measurements of Capella with the Low-Energy Transmission Grating Spectrometer aboard the Chandra X-Ray Observatory
Published in The Astrophysical journal (20-02-2000)“…We present the first X-ray spectrum obtained by the Low-Energy Transmission Grating Spectrometer (LETGS) aboard the Chandra X-Ray Observatory. The spectrum is…”
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The X-ray spectra of the flaring and quiescent states of YZ CMi observed by XMM–Newton
Published in Monthly notices of the Royal Astronomical Society (11-08-2007)“…We analyse the X-ray spectrum of the active late-type star YZ CMi (M4.5V); for quiescent as well as active stages, we derive emission measure (EM)…”
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A COMPREHENSIVE X-RAY ABSORPTION MODEL FOR ATOMIC OXYGEN
Published in The Astrophysical journal (10-12-2013)“…An analytical formula is developed to accurately represent the photoabsorption cross section of O I for all energies of interest in X-ray spectral modeling. In…”
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Spectra of Ni V and Fe V in the Vacuum Ultraviolet
Published 12-11-2019“…This work presents 97 remeasured Fe V wavelengths (1200 \r{A} to 1600 \r{A}) and 123 remeasured Ni V wavelengths (1200 \r{A} to 1400 \r{A}) with uncertainties…”
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X-ray spectra of the Fe-L complex III: systematic uncertainties in the atomic data
Published 14-06-2022“…A&A 664, A62 (2022) There has been a growing request from the X-ray astronomy community for a quantitative estimate of systematic uncertainties originating…”
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Magnesium and silicon in interstellar dust: an X-ray overview
Published 07-07-2020“…A&A 641, A149 (2020) The dense Galactic environment is a large reservoir of interstellar dust. Therefore, this region represents a perfect laboratory to study…”
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X-ray spectra of the Fe-L complex
Published 20-05-2019“…A&A 627, A51 (2019) The Hitomi results on the Perseus cluster lead to improvements in our knowledge of atomic physics which are crucial for the precise…”
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11
Charge exchange in galaxy clusters
Published 13-10-2017“…A&A 611, A26 (2018) Though theoretically expected, the charge exchange emission from galaxy clusters has not yet been confidently detected. Accumulating hints…”
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X-ray spectra of the Fe-L complex II: atomic data constraints from EBIT experiment and X-ray grating observations of Capella
Published 08-07-2020“…A&A 641, A93 (2020) The Hitomi results for the Perseus cluster have shown that accurate atomic models are essential to the success of X-ray spectroscopic…”
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13
Plasma code for astrophysical charge exchange emission at X-ray wavelengths
Published 22-01-2016“…A&A 588, A52 (2016) Charge exchange X-ray emission provides unique insights into the interactions between cold and hot astrophysical plasmas. Besides its own…”
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Density diagnostics of ionized outflows in active galactic nuclei: X-ray and UV absorption lines from metastable levels in Be-like to C-like ions
Published 15-08-2017“…A&A 607, A100 (2017) Ionized outflows in Active Galactic Nuclei (AGN) are thought to influence their nuclear and local galactic environment. However, the…”
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15
Line absorption of He-like triplet lines by Li-like ions. Caveats of using line ratios of triplets for plasma diagnostics
Published 03-06-2015“…A&A 579, A87 (2015) He-like ions produce distinctive series of triplet lines under various astrophysical conditions. However, this emission can be affected by…”
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Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi
Published in Publications of the Astronomical Society of Japan (01-03-2018)“…Abstract The Hitomi Soft X-ray Spectrometer spectrum of the Perseus cluster, with ∼5 eV resolution in the 2–9 keV band, offers an unprecedented benchmark of…”
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Science with hot astrophysical plasmas
Published 05-07-2017“…We present some recent highlights and prospects for the study of hot astrophysical plasmas. Hot plasmas can be studied primarily through their X-ray emission…”
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The X-ray spectrum of delta Orionis observed by LETGS aboard Chandra
Published 09-01-2013“…A&A, 550, 55 (2013) We analyze the high-resolution X-ray spectrum of the supergiant O-star delta Orionis (O9.5II) with line ratios of He-like ions and a…”
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A novel scenario for the possible X-ray line feature at ~3.5 keV: Charge exchange with bare sulfur ions
Published 20-11-2015“…Motivated by recent claims of a compelling ~3.5 keV emission line from nearby galaxies and galaxy clusters, we investigate a novel plasma model incorporating a…”
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Calibration and in orbit performance of the reflection grating spectrometer onboard XMM-Newton
Published 20-10-2014“…A&A 573, A128 (2015) Context: XMM-Newton was launched on 10 December 1999 and has been operational since early 2000. One of the instruments onboard XMM-Newton…”
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