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Context. The radiation field consisting of hydrogen recombination lines and continuum emission might significantly affect the hydrogen-level populations in ultra- and hypercompact (U/HC) H II regions. The escape probability approximation…

星系天体物理 · 物理学 2025-09-17 F. -Y. Zhu , J. Wang , Y. Qiu , Q. -F. Zhu , D. Quan

The discovery of the first naturally occurring high gain hydrogen recombination line (HRL) maser, in the millimeter and submillimeter spectrum of the emission line star MWC349, requires an expansion of current paradigms about HRLs. In this…

天体物理学 · 物理学 2012-08-27 Vladimir S. Strelnitski , Victor O. Ponomarev , Howard A. Smith

At intermediate to high densities, electron (de-)excitation collisions are the dominant process for populating or depopulating high Rydberg states. In particular, the accurate knowledge of the energy changing ($n$-changing) collisional…

星系天体物理 · 物理学 2019-04-10 F. Guzmán , M. Chatzikos , P. A. M. van Hoof , Dana S. Balser , M. Dehghanian , N. R. Badnell , G. J. Ferland

The importance of some atom hydrogen collisions in AGN has been investigated. The results are useful for better estimate of the hydrogen Balmer lines uxes, which usage for effective temperature diagnostics in astrophysical plasma is limited…

星系天体物理 · 物理学 2020-01-15 M. S. Dimitrijevic , V. A. Sreckovic , Lj. M. Ignjatovic , B. P. Marinkovic

Nuclear materials are often demanded to function for extended time in extreme environments, including high radiation fluxes and transmutation, high temperature and temperature gradients, stresses, and corrosive coolants. They also have a…

材料科学 · 物理学 2022-11-18 Dane Morgan , Ghanshyam Pilania , Adrien Couet , Blas P. Uberuaga , Cheng Sun , Ju Li

Radiative transfer in hydrogen lines in supernova remnant (SNR) shock waves is studied taking into account the population of the hydrogen atom 2s-state. Measurements of Balmer line emission, especially of H~$\alpha$, are often relied upon…

高能天体物理现象 · 物理学 2019-03-27 Jiro Shimoda , J. Martin Laming

Hydrogen recombination lines are one of the major diagnostics of H II region physical properties and kinematics. In the near future, the Expanded Very Large Array (EVLA) and the Atacama Large Millimeter Array (ALMA) will allow observers to…

星系天体物理 · 物理学 2012-09-04 Thomas Peters , Steven N. Longmore , Cornelis P. Dullemond

We survey the results of a long-term study of the process of radiative recombination. A rigorous theory of nonrelativistic electron radiative recombination with a hydrogen-like ion is used to calculate the total cross section of the…

原子物理 · 物理学 2019-03-27 Igor A. Kotelnikov , Alexander I. Milstein

The recombination model as a model for hadronization from a quark-gluon plasma has been recently revived since it has advantages in explaining several important features of the final state produced in heavy-ion collisions at RHIC, such as…

核理论 · 物理学 2010-01-15 Kang Seog Lee , Steffen Bass , Berndt Mueller , Chiho Nonaka

Previous radio recombination line (RRL) observations of dust clumps identified in the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) have led to the detection of a large number of RRLs in the 3mm range. Here, we aim to study…

星系天体物理 · 物理学 2018-08-29 W. -J. Kim , J. S. Urquhart , F. Wyrowski , K. M. Menten , T. Csengeri

The helium I line intensity ratio (LIR) method is used to measure the electron density ($n_e$) and temperature ($T_e$) of fusion-relevant plasmas. Although the collisional-radiative model (CRM) has been used to predict $n_e$ and $T_e$,…

等离子体物理 · 物理学 2025-06-26 Shin Kajita

Hydrogen and helium emission lines in nebulae form by radiative recombination. This is a simple process which, in principle, can be described to very high precision. Ratios of He I and H I emission lines can be used to measure the…

星系天体物理 · 物理学 2016-04-27 F. Guzmán , N. R. Badnell , R. J. R. Williams , P. A. M. van Hoof , M. Chatzikos , G. J. Ferland

A model for ionization and recombination collisions in a multifluid plasma is formulated using the framework introduced in previous work [{Phys. Plasmas} \textbf{22}, 093512 (2015)]. The exchange source terms for density, momentum and…

等离子体物理 · 物理学 2016-06-22 H. P. Le , J. -L. Cambier

We report the detection of a new radio recombination line (RRL) maser object toward the IRS2 source in the MonR2 ultracompact HII region. The continuum emission at 1.3mm and 0.85mm and the H30a and H26a lines were observed with the…

太阳与恒星天体物理 · 物理学 2015-06-12 I. Jimenez-Serra , A. Baez-Rubio , V. M. Rivilla , J. Martin-Pintado , Q. Zhang , M. Dierickx , N. Patel

Quantitative spectroscopy of molecular hydrogen has generated substantial demand, leading to the accumulation of diverse elementary-process data encompassing radiative transitions, electron-impact transitions, predissociations, and…

HII regions made of gas ionized by radiations from young massive stars, are widely distributed in the Milky Way. They are tracers for star formation, and their distributions are correlated with the Galactic spiral structure. Radio…

星系天体物理 · 物理学 2021-11-03 Chuan-Peng Zhang , Jin-Long Xu , Guang-Xing Li , Li-Gang Hou , Nai-Ping Yu , Peng Jiang

The Glauber model is extensively applied to heavy ion collision for describing a number of interaction processes over a wide range of energies from near the Coulomb barrier to higher energies. The model gives the nucleus-nucleus interaction…

核理论 · 物理学 2007-05-23 P. Shukla

This work presents a few preliminary results from a collisional-radiative (CR) model intended to describe an argon microwave (2.45 GHz) plasma at atmospheric pressure. This model aims to investigate the influence of dissociative…

等离子体物理 · 物理学 2007-05-23 Abel Sainz , Joelle Margot , Maria Carmen Garcia , Maria Dolores Calzada

We revisit the Glauber model to study the heavy ion reaction cross sections and elastic scattering angular distributions at low and intermediate energies. The Glauber model takes nucleon-nucleon cross sections and nuclear densities as…

核理论 · 物理学 2017-04-26 Ajay Mehndiratta , Prashant Shukla

This paper presents a study of the dependence of the simulated intensities of recombination lines from hydrogen and helium atoms on the number of $n\ell$-resolved principal quantum numbers included in the calculations. We simulate hydrogen…

星系天体物理 · 物理学 2025-04-15 F. Guzmán , M. Chatzikos , G. Ferland
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