English
Related papers

Related papers: X-ray emission measurements following charge excha…

200 papers

We report results of a theoretical investigation of polarization of the X-ray emissions induced in charge-exchange collisions of fully stripped solar wind ions C$^{6+}$ and O$^{8+}$ with the heliospheric hydrogen atoms. The polarization of…

Earth and Planetary Astrophysics · Physics 2013-11-14 Marko Gacesa , Hans-Reinhard Müller , Robin Côté , Vasili Kharchenko

Measurements of [OIII] emission in Lyman Break galaxies (LBGs) at z>3 are presented. Four galaxies were observed with narrow-band filters using the Near-IR Camera on the Keck I 10-m telescope. A fifth galaxy was observed spectroscopically…

The introduction of gases like nitrogen or neon for cooling the edge region of magnetically confined fusion plasmas has triggered a renewed interest in state selective cross sections necessary for plasma diagnostics by means of charge…

We investigate the energy dependence and the internal-state dependence of the charge-exchange collision cross sections in a mixture of $^6$Li atoms and $^{40}$Ca$^+$ ions in the collision energy range from 0.2 mK to 1 K. Deliberately…

Atomic Physics · Physics 2017-04-05 R. Saito , S. Haze , M. Sasakawa , R. Nakai , M. Raoult , H. Da Silva , O. Dulieu , T. Mukaiyama

The past decade has seen a surge of interest in astrophysical charge exchange (CX). The impetus was the discovery of X-ray emission from comets in 1996, soon followed by the observation of CX emission in planetary atmospheres and throughout…

Astrophysics · Physics 2009-11-13 B. J. Wargelin , P. Beiersdorfer , G. V. Brown

Charge exchange between highly charged ions and neutral atoms and molecules has been considered as one of the important mechanisms controlling soft X ray emissions in many astrophysical objects and environments. However, for modeling charge…

Astrophysics of Galaxies · Physics 2021-05-11 J. W. Xu , C. X. Xu , R. T. Zhang , X. L. Zhu , W. T. Feng , L. Gu , G. Y. Liang , D. L. Guo , Y. Gao , D. M. Zhao , S. F. Zhang , M. G. Su , X. Ma

This paper reports on a search for flare emission via charge-exchange radiation in the wings of the Lyman-alpha line of He ii at 304 A, as originally suggested for hydrogen by Orrall and Zirker. Via this mechanism a primary alpha particle…

Solar and Stellar Astrophysics · Physics 2014-01-28 Hugh Hudson , Lyndsay Fletcher , Alec MacKinnon , Tom Woods

Double photoelectron emission from He atoms by intense laser pulses with a wave length of $394.5\,nm$ is computed for intensities $3.5 - 9.2\times 10^{14}W/cm^2$. Joint momentum distributions confirm the characteristics seen in classical…

Atomic Physics · Physics 2020-07-01 Jinzhen Zhu , Armin Scrinzi

Recent X-ray studies have shown that supernova shock models are unable to satisfactorily explain X-ray emission in the rim of the Cygnus Loop. In an attempt to account for this anomalously enhanced X-ray flux, we fit the region with a model…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Renata S. Cumbee , David B. Henley , Phillip C. Stancil , Robin L. Shelton , Jeff L. Nolte , Yong Wu , David R. Schultz

We study the x-ray emission following the collision of a Bi$^{83+}$ ion with a neutral Xe atom at the projectile energy 70 MeV/u. The collisional and post-collisional processes are treated separately. The probabilities of various…

We present measurements of K-shell x-ray emission following charge exchange of fully ionized argon with various neutral gaseous targets at small collision energies inside an electron beam ion trap. We also resolve the principal quantum…

Charge exchange (CX) has emerged in X-ray emission modeling as a significant process that must be considered in many astrophysical environment--particularly comets. Comets host an interaction between solar wind ions and cometary neutrals to…

High Energy Astrophysical Phenomena · Physics 2017-07-31 P. D. Mullen , R. S. Cumbee , D. Lyons , L. Gu , J. Kaastra , R. L. Shelton , P. C. Stancil

It has been proposed that the charge exchange (CX) process at the interface between hot and cool interstellar gases could contribute significantly to the observed soft X-ray emission in star forming galaxies. We analyze the XMM-Newton/RGS…

Astrophysics of Galaxies · Physics 2015-06-22 Shuinai Zhang , Q. Daniel Wang , Li Ji , Randall K. Smith , Adam R. Foster , Xin Zhou

We present an XMM-Newton spectrum of diffuse X-ray emission from within the solar system. The spectrum is dominated by probable C VI lines at 0.37 keV and 0.46 keV, an O VII line at 0.56 keV, O VIII lines at 0.65 keV and ~0.8 keV, Ne IX…

Astrophysics · Physics 2009-11-10 S. L. Snowden , M. R. Collier , K. D. Kuntz

For bare lead ions, decelerated to the low beam energy of 10 MeV/u, the x-ray emission associated with radiative recombination (RR) at "cold collision" conditions has been studied at the electron cooler of CRYRING@ESR at GSI-Darmstadt.…

Transition edge sensor microcalorimeters can measure x-ray and gamma-ray energies with very high energy resolution and high photon-collection efficiency. For this technology to reach its full potential in future x-ray observatories, each…

Instrumentation and Methods for Astrophysics · Physics 2017-02-03 J. W. Fowler , B. K. Alpert , W. B. Doriese , D. A. Fischer , C. Jaye , Y. I. Joe , G. C. O'Neil , D. S. Swetz , J. N. Ullom

We present observations of the Lyman alpha forest towards B2 1225+317 taken at a resolution of 18 km/s. A clean sample of Lyman alpha forest lines is extracted after a careful profile fitting analysis and removal of absorption lines of…

Astrophysics · Physics 2015-06-24 Pushpa Khare , R. Srianand , D. G. York , R. Green , D. Welty , Ke-Liang Huang , J. Bechtold

We present a study of Lyman continuum (LyC) emission in a sample of $\sim$150 Ly$\alpha$ emitters (LAEs) at $z\approx3.1$ in the Subaru-XMM Deep Survey field. These LAEs were previously selected using the narrowband technique and…

Astrophysics of Galaxies · Physics 2023-10-12 Yuchen Liu , Linhua Jiang , Rogier A. Windhorst , Yucheng Guo , Zhenya Zheng

We report new measurements of the drift velocity and longitudinal diffusion coefficients of electrons in pure xenon gas and in xenon-helium gas mixtures at 1-9 bar and electric field strengths of 50-300 V/cm. In pure xenon we find excellent…

Future microcalorimeter X-ray observations will resolve spectral features in unmatched detail. Understanding the line formation processes in the X-rays deserves much attention. The purpose of this paper is to discuss such processes in the…

High Energy Astrophysical Phenomena · Physics 2021-05-12 Priyanka Chakraborty , Gary Ferland , Marios Chatzikos , Francisco Guzmán , Yuanyuan Su