Simulation of Line Profiles of the Krypton Spectra Emitted by the Plasma of Current Sheets
Sign Up to like & getrecommendations! Published in 2019 at "Russian Physics Journal"
DOI: 10.1007/s11182-019-01666-3
Abstract: Line profiles of the krypton spectra emitted by the plasma of current sheets are simulated. Current sheets are formed under the impact of magnetic fields with singular X-lines. The spectral line profiles are calculated by… read more here.
Keywords: line profiles; krypton spectra; current sheets; profiles krypton ... See more keywords
Radiative transfer modeling of the observed line profiles in G31.41+0.31
Sign Up to like & getrecommendations! Published in 2021 at "Advances in Space Research"
DOI: 10.1016/j.asr.2021.07.011
Abstract: An inverse P-Cygni profile of H13CO+ (1 → 0) in G31.41+0.31 was recently observed, which indicates the presence of an infalling gas envelope. Also, an outflow tracer, SiO, was observed. Here, exclusive radiative transfer modelings… read more here.
Keywords: line; observed line; gas; line profiles ... See more keywords
LIFELINE: The program for the simulation of the X-ray line profiles in massive colliding wind binaries
Sign Up to like & getrecommendations! Published in 2020 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/202039437
Abstract: The study of the X-ray line profiles produced by massive colliding wind binaries is a powerful tool for the characterisation of the stellar winds. We built a self-consistent program for the computation of line profiles… read more here.
Keywords: massive colliding; wind; line; ray line ... See more keywords
Forbidden line diagnostics of photoevaporative disc winds
Sign Up to like & getrecommendations! Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa1767
Abstract: Photoevaporation driven by high energy radiation from the central star plays an important role in the evolution of protoplanetary discs. Photoevaporative winds have been unambiguously detected through blue-shifted emission lines, but their detailed properties remain… read more here.
Keywords: disc winds; disc; emission lines; line ... See more keywords