Spectral line analysis: voigt profile of a, k and g stars, general and empirical curve of growth and abundance of elements in m,f,k and g stars using lte formalism
The study of spectra has revealed properties of matter and has allowed us to understand more about the universe we live in. To the same extent, it grasps a huge variety of fields of study like physics, chemistry and astrophysics among others. By taking spectra samples (the finger print of the stella...
- Autores:
-
Savino Gómez, Laura
- Tipo de recurso:
- Trabajo de grado de pregrado
- Fecha de publicación:
- 2006
- Institución:
- Universidad de los Andes
- Repositorio:
- Séneca: repositorio Uniandes
- Idioma:
- eng
- OAI Identifier:
- oai:repositorio.uniandes.edu.co:1992/76141
- Acceso en línea:
- https://hdl.handle.net/1992/76141
- Palabra clave:
- Análisis espectral
Equilibrio termodinámico
Radiación cósmica
Física
- Rights
- openAccess
- License
- http://purl.org/coar/access_right/c_abf2
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Spectral line analysis: voigt profile of a, k and g stars, general and empirical curve of growth and abundance of elements in m,f,k and g stars using lte formalism |
| title |
Spectral line analysis: voigt profile of a, k and g stars, general and empirical curve of growth and abundance of elements in m,f,k and g stars using lte formalism |
| spellingShingle |
Spectral line analysis: voigt profile of a, k and g stars, general and empirical curve of growth and abundance of elements in m,f,k and g stars using lte formalism Análisis espectral Equilibrio termodinámico Radiación cósmica Física |
| title_short |
Spectral line analysis: voigt profile of a, k and g stars, general and empirical curve of growth and abundance of elements in m,f,k and g stars using lte formalism |
| title_full |
Spectral line analysis: voigt profile of a, k and g stars, general and empirical curve of growth and abundance of elements in m,f,k and g stars using lte formalism |
| title_fullStr |
Spectral line analysis: voigt profile of a, k and g stars, general and empirical curve of growth and abundance of elements in m,f,k and g stars using lte formalism |
| title_full_unstemmed |
Spectral line analysis: voigt profile of a, k and g stars, general and empirical curve of growth and abundance of elements in m,f,k and g stars using lte formalism |
| title_sort |
Spectral line analysis: voigt profile of a, k and g stars, general and empirical curve of growth and abundance of elements in m,f,k and g stars using lte formalism |
| dc.creator.fl_str_mv |
Savino Gómez, Laura |
| dc.contributor.advisor.none.fl_str_mv |
Oostra Vannoppen, Benjamín |
| dc.contributor.author.none.fl_str_mv |
Savino Gómez, Laura |
| dc.subject.keyword.none.fl_str_mv |
Análisis espectral Equilibrio termodinámico Radiación cósmica |
| topic |
Análisis espectral Equilibrio termodinámico Radiación cósmica Física |
| dc.subject.themes.spa.fl_str_mv |
Física |
| description |
The study of spectra has revealed properties of matter and has allowed us to understand more about the universe we live in. To the same extent, it grasps a huge variety of fields of study like physics, chemistry and astrophysics among others. By taking spectra samples (the finger print of the stellar objects), one may determine quantum effects and composition of the sample to be analyzed. Through the information inside each spectra we may determine the age of stars -wheather stars have a planetary system or are acompained by other stars (binary systems)-, or if they are the result of the evolution of early supernovas. As you may infer, the application of the study of spectra is astronomical. Throughout my work, I attend to show how to calculate abundance of chemical elements in stars. |
| publishDate |
2006 |
| dc.date.issued.none.fl_str_mv |
2006-11-29 |
| dc.date.accessioned.none.fl_str_mv |
2025-04-09T15:37:22Z |
| dc.date.available.none.fl_str_mv |
2025-04-09T15:37:22Z |
| dc.type.none.fl_str_mv |
Trabajo de grado - Pregrado |
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info:eu-repo/semantics/bachelorThesis |
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https://hdl.handle.net/1992/76141 |
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instname:Universidad de los Andes |
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reponame:Repositorio Institucional Séneca |
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https://hdl.handle.net/1992/76141 |
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eng |
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eng |
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openAccess |
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43 páginas |
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application/pdf |
| dc.publisher.none.fl_str_mv |
Universidad de los Andes |
| dc.publisher.program.none.fl_str_mv |
Física |
| dc.publisher.faculty.none.fl_str_mv |
Facultad de Ciencias |
| dc.publisher.department.none.fl_str_mv |
Departamento de Física |
| publisher.none.fl_str_mv |
Universidad de los Andes |
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Universidad de los Andes |
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Oostra Vannoppen, Benjamínvirtual::24030-1Savino Gómez, Laura2025-04-09T15:37:22Z2025-04-09T15:37:22Z2006-11-29https://hdl.handle.net/1992/76141instname:Universidad de los Andesreponame:Repositorio Institucional Sénecarepourl:https://repositorio.uniandes.edu.co/The study of spectra has revealed properties of matter and has allowed us to understand more about the universe we live in. To the same extent, it grasps a huge variety of fields of study like physics, chemistry and astrophysics among others. By taking spectra samples (the finger print of the stellar objects), one may determine quantum effects and composition of the sample to be analyzed. Through the information inside each spectra we may determine the age of stars -wheather stars have a planetary system or are acompained by other stars (binary systems)-, or if they are the result of the evolution of early supernovas. As you may infer, the application of the study of spectra is astronomical. Throughout my work, I attend to show how to calculate abundance of chemical elements in stars.Pregrado43 páginasapplication/pdfengUniversidad de los AndesFísicaFacultad de CienciasDepartamento de FísicaSpectral line analysis: voigt profile of a, k and g stars, general and empirical curve of growth and abundance of elements in m,f,k and g stars using lte formalismTrabajo de grado - Pregradoinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_7a1fTexthttp://purl.org/redcol/resource_type/TPAnálisis espectralEquilibrio termodinámicoRadiación cósmicaFísicainfo:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Publication0000-0002-1288-7978virtual::24030-1https://scienti.minciencias.gov.co/cvlac/visualizador/generarCurriculoCv.do?cod_rh=0000230731virtual::24030-15187476c-bab7-4535-bced-104b06c4401bvirtual::24030-15187476c-bab7-4535-bced-104b06c4401bvirtual::24030-1LICENSElicense.txtlicense.txttext/plain; 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