Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries

Detalhes bibliográficos
Autor(a) principal: Pelisoli, Ingrid Domingos
Data de Publicação: 2015
Outros Autores: Santos, Marcio Gabriel dos, Kepler, Souza Oliveira
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/115355
Resumo: We present new calculations of unified line profiles for hydrogen perturbed by collisions with protons. We report on new calculations of the potential energies and dipole moments which allow the evaluation of profiles for the lines of the Lyman series up to Lyman δ and the Balmer series up to Balmer 10. Unified calculations only existed for the lines Lyman α to Lyman γ and Balmer α including the H+ 2 quasi-molecule. These data are available as online material accompanying this paper and should be included in atmosphere models, in place of the Stark effect of protons, since the quasi-molecular contributions cause not only satellites, but large asymmetries that are unaccounted for in models that assume that Stark broadening of electrons and that of protons are equal.
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spelling Pelisoli, Ingrid DomingosSantos, Marcio Gabriel dosKepler, Souza Oliveira2015-04-15T01:58:22Z20150035-8711http://hdl.handle.net/10183/115355000955058We present new calculations of unified line profiles for hydrogen perturbed by collisions with protons. We report on new calculations of the potential energies and dipole moments which allow the evaluation of profiles for the lines of the Lyman series up to Lyman δ and the Balmer series up to Balmer 10. Unified calculations only existed for the lines Lyman α to Lyman γ and Balmer α including the H+ 2 quasi-molecule. These data are available as online material accompanying this paper and should be included in atmosphere models, in place of the Stark effect of protons, since the quasi-molecular contributions cause not only satellites, but large asymmetries that are unaccounted for in models that assume that Stark broadening of electrons and that of protons are equal.application/pdfengMonthly notices of the royal astronomical society. Oxford [recurso eletrônico]. Vol. 448, n. 3 (April 2015), p. 2332-2343Anãs brancasHidrogênioPrótonsSatélitesAtomic dataLine: profilesWhite dwarfsUnified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetriesEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSORIGINAL000955058.pdf000955058.pdfTexto completo (inglês)application/pdf3759592http://www.lume.ufrgs.br/bitstream/10183/115355/1/000955058.pdfd9673535119179dcad2f318850abc27aMD51TEXT000955058.pdf.txt000955058.pdf.txtExtracted Texttext/plain56870http://www.lume.ufrgs.br/bitstream/10183/115355/2/000955058.pdf.txt5cc53f2a55e842d838a88696ad57bbe0MD52THUMBNAIL000955058.pdf.jpg000955058.pdf.jpgGenerated Thumbnailimage/jpeg2087http://www.lume.ufrgs.br/bitstream/10183/115355/3/000955058.pdf.jpg511b5e0215d456b7f7d0b9da3319bb05MD5310183/1153552022-06-17 04:47:17.847584oai:www.lume.ufrgs.br:10183/115355Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2022-06-17T07:47:17Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
title Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
spellingShingle Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
Pelisoli, Ingrid Domingos
Anãs brancas
Hidrogênio
Prótons
Satélites
Atomic data
Line: profiles
White dwarfs
title_short Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
title_full Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
title_fullStr Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
title_full_unstemmed Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
title_sort Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
author Pelisoli, Ingrid Domingos
author_facet Pelisoli, Ingrid Domingos
Santos, Marcio Gabriel dos
Kepler, Souza Oliveira
author_role author
author2 Santos, Marcio Gabriel dos
Kepler, Souza Oliveira
author2_role author
author
dc.contributor.author.fl_str_mv Pelisoli, Ingrid Domingos
Santos, Marcio Gabriel dos
Kepler, Souza Oliveira
dc.subject.por.fl_str_mv Anãs brancas
Hidrogênio
Prótons
Satélites
topic Anãs brancas
Hidrogênio
Prótons
Satélites
Atomic data
Line: profiles
White dwarfs
dc.subject.eng.fl_str_mv Atomic data
Line: profiles
White dwarfs
description We present new calculations of unified line profiles for hydrogen perturbed by collisions with protons. We report on new calculations of the potential energies and dipole moments which allow the evaluation of profiles for the lines of the Lyman series up to Lyman δ and the Balmer series up to Balmer 10. Unified calculations only existed for the lines Lyman α to Lyman γ and Balmer α including the H+ 2 quasi-molecule. These data are available as online material accompanying this paper and should be included in atmosphere models, in place of the Stark effect of protons, since the quasi-molecular contributions cause not only satellites, but large asymmetries that are unaccounted for in models that assume that Stark broadening of electrons and that of protons are equal.
publishDate 2015
dc.date.accessioned.fl_str_mv 2015-04-15T01:58:22Z
dc.date.issued.fl_str_mv 2015
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10183/115355
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dc.language.iso.fl_str_mv eng
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dc.relation.ispartof.pt_BR.fl_str_mv Monthly notices of the royal astronomical society. Oxford [recurso eletrônico]. Vol. 448, n. 3 (April 2015), p. 2332-2343
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