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Spatially resolved plasma diagnostics of the supernova remnant DEM L71 using the reflection grating spectrometer
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High-resolution X-ray spectra of the compact binary supersoft X-ray source CAL 87
The Rockets for Extended-source X-ray Spectroscopy Instrument Design
Drew M. Miles, Randall L. McEntaffer, James H. Tutt, Logan Baker, Ross McCurdy, Bailey Myers, Bridget O’Meara and Joseph Weston The Astrophysical Journal 971(2) 171 (2024) https://doi.org/10.3847/1538-4357/ad58d4
Revealing the burning and soft heart of the bright bare active galactic nucleus ESO 141-G55: X-ray broadband and SED analysis
Doppler Broadening and Line-of-sight Effects in Core-collapse Supernovae and Young Remnants
Taylor Jacovich, Daniel Patnaude, Patrick Slane, Carles Badenes, Shiu-Hang Lee, Shigehiro Nagataki and Dan Milisavljevic The Astrophysical Journal 951(1) 57 (2023) https://doi.org/10.3847/1538-4357/acd0ad
Theoretical study of dielectronic recombination and electron-impact excitation for helium-like isoelectronic sequence
Support for the standard picture of thermal X-rays in the wind of ζ Puppis from dielectronic recombination of He-like ions
Sean J Gunderson, Kenneth G Gayley and David P Huenemoerder Monthly Notices of the Royal Astronomical Society 522(2) 2739 (2023) https://doi.org/10.1093/mnras/stad1163
Abundance and temperature of the outer hot circumgalactic medium
G. Ponti, X. Zheng, N. Locatelli, S. Bianchi, Y. Zhang, K. Anastasopoulou, J. Comparat, K. Dennerl, M. Freyberg, F. Haberl, A. Merloni, T. H. Reiprich, M. Salvato, J. Sanders, M. Sasaki, A. Strong and M. C. H. Yeung Astronomy & Astrophysics 674 A195 (2023) https://doi.org/10.1051/0004-6361/202243992
Helium-like X-ray line complexes show that the hottest plasma on the O supergiant ζ Puppis is in its wind
David H Cohen, Ariel M Overdorff, Maurice A Leutenegger, Marc Gagné, Véronique Petit and Alexandre David-Uraz Monthly Notices of the Royal Astronomical Society 513(2) 1609 (2022) https://doi.org/10.1093/mnras/stac899
Understanding the physical state of hot plasma formed through stellar wind collision in WR140 using high-resolution X-ray spectroscopy
Asca Miyamoto, Yasuharu Sugawara, Yoshitomo Maeda, et al. Monthly Notices of the Royal Astronomical Society 513(4) 6074 (2022) https://doi.org/10.1093/mnras/stac1289
The X-ray Emission of γ Cassiopeiae During the 2020–2021 disc eruption
Satellite lines of helium-like ions in strongly coupled plasma environment
R. Chandra, S. Bhattacharyya, J.K. Saha, X. Li and T.K. Mukherjee Journal of Quantitative Spectroscopy and Radiative Transfer 272 107830 (2021) https://doi.org/10.1016/j.jqsrt.2021.107830
Calculations of Dielectronic Recombination and Electron-impact Excitation Rate Coefficients of Highly Charged Sulfur Ions
D. H. Zhang, Z. W. Wu, C. Ren, J. Jiang, L. Y. Xie, R. Schuch, J. M. Zhang and C. Z. Dong The Astrophysical Journal Supplement Series 247(1) 22 (2020) https://doi.org/10.3847/1538-4365/ab6b2c
X-ray evolution of the nova V959 Mon suggests a delayed ejection and a non-radiative shock
Thomas Nelson, Koji Mukai, Laura Chomiuk, et al. Monthly Notices of the Royal Astronomical Society 500(3) 2798 (2020) https://doi.org/10.1093/mnras/staa3367
High-resolution X-ray spectroscopy of the stellar wind in Vela X-1 during a flare
Soft X-ray emission lines in the X-ray binary Swift J1858.6–0814 observed with XMM–Newton Reflection Grating Spectrometer: disc atmosphere or wind?
D J K Buisson, D Altamirano, M Díaz Trigo, et al. Monthly Notices of the Royal Astronomical Society 498(1) 68 (2020) https://doi.org/10.1093/mnras/staa2258
Variability in X-ray line ratios in helium-like ions of massive stars: the wind-driven case
Laboratory measurements of geometrical effects in the x-ray emission of optically thick lines for ICF diagnostics
G. Pérez-Callejo, L. C. Jarrott, D. A. Liedahl, E. V. Marley, G. E. Kemp, R. F. Heeter, J. A. Emig, M. E. Foord, K. Widmann, J. Jaquez, H. Huang, S. J. Rose, J. S. Wark and M. B. Schneider Physics of Plasmas 26(6) (2019) https://doi.org/10.1063/1.5096972
ROME (Radio Observations of Magnetized Exoplanets). II. HD 189733 Does Not Accrete Significant Material from Its Exoplanet Like a T Tauri Star from a Disk
Probing the Hot X-Ray Gas in the Narrow-line Region of Mrk 3
Ákos Bogdán, Ralph P. Kraft, Daniel A. Evans, Felipe Andrade-Santos and William R. Forman The Astrophysical Journal 848(1) 61 (2017) https://doi.org/10.3847/1538-4357/aa8c76
On the Binary Nature of Massive Blue Hypergiants: High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12 is a Colliding Wind Binary
L. M. Oskinova, D. P. Huenemoerder, W.-R. Hamann, T. Shenar, A. A. C. Sander, R. Ignace, H. Todt and R. Hainich The Astrophysical Journal 845(1) 39 (2017) https://doi.org/10.3847/1538-4357/aa7e79
The clumpy absorber in the high-mass X-ray binary Vela X-1
Thermal X-ray emission from a baryonic jet: a self-consistent multicolour spectral model
I. Khabibullin, P. Medvedev and S. Sazonov Monthly Notices of the Royal Astronomical Society 455(2) 1414 (2016) https://doi.org/10.1093/mnras/stv2432
Moving inhomogeneous envelopes of stars
Lidia M. Oskinova, Brankica Kubátová and Wolf-Rainer Hamann Journal of Quantitative Spectroscopy and Radiative Transfer 183 100 (2016) https://doi.org/10.1016/j.jqsrt.2016.06.017
Energy levels and transition rates for helium-like ions withZ = 10–36
X-ray, UV and optical analysis of supergiants: ϵ Ori
Raul E. Puebla, D. John Hillier, Janos Zsargó, David H. Cohen and Maurice A. Leutenegger Monthly Notices of the Royal Astronomical Society 456(3) 2907 (2016) https://doi.org/10.1093/mnras/stv2783
A benchmark of the He-like triplet for ions with 6 ≤Z≤ 14 in Maxwellian and non-Maxwellian plasmas
Y. Rodríguez, E. Gatuzz, M. A. Bautista and C. Mendoza Monthly Notices of the Royal Astronomical Society 461(2) 1374 (2016) https://doi.org/10.1093/mnras/stw1384
CHEMICAL AND PHYSICAL PARAMETERS FROM X-RAY HIGH-RESOLUTION SPECTRA OF THE GALACTIC NOVA V959 MON
U. Peretz, M. Orio, E Behar, A. Bianchini, J. Gallagher, T. Rauch, B. Tofflemire and P. Zemko The Astrophysical Journal 829(1) 2 (2016) https://doi.org/10.3847/0004-637X/829/1/2
Plasma-screening effects in the astrophysically relevant He-like
and Li-like Mg and Fe ions*
Validation of x-ray line ratios for electron temperature determination in tokamak plasmas
A S Rosen, M L Reinke, J E Rice, A E Hubbard and J W Hughes Journal of Physics B: Atomic, Molecular and Optical Physics 47(10) 105701 (2014) https://doi.org/10.1088/0953-4075/47/10/105701
DN Tauri – coronal activity and accretion in a young low-mass CTTS
Hyperfine quenching of the metastable 4s4p 3P0 and 3P2 states of Zn-like ions1This article is part of a Special Issue on the 10th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas.