Detalhes bibliográficos
| Ano de defesa: |
2018 |
| Autor(a) principal: |
Santana, Paulo Henrique Gomes
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| Orientador(a): |
Fernandes, Iranderly Fernandes
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| Banca de defesa: |
Não Informado pela instituição |
| Tipo de documento: |
Dissertação
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| Tipo de acesso: |
Acesso aberto |
| Idioma: |
por |
| Instituição de defesa: |
Universidade Estadual de Feira de Santana
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| Programa de Pós-Graduação: |
Mestrado em Computação Aplicada
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| Departamento: |
DEPARTAMENTO DE TECNOLOGIA
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| País: |
Brasil
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| Palavras-chave em Português: |
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| Palavras-chave em Inglês: |
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| Área do conhecimento CNPq: |
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| Link de acesso: |
http://tede2.uefs.br:8080/handle/tede/729
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Resumo: |
The aim of this work is to mimic the spectroscopic observation carried in a telescope with a diffraction gap, or with optical fiber of extensive astronomic objects, using the codes of computational simulation – which were created to reproduce the physical and chemical conditions of the regions – to obtain this effect. The studied regions were the Planetary Nebulae. So, in this research the photoionization code used was Cloudy because it simulates the radioactive processes of Planetary Nebulae, creating synthetic spectrums to mime a real spectrum. In these spectrums we studied the intensity of the spectral lines responsible for the cooling of the cloud, namely: ([OI] 6300 Å)/(Hβ 4861 Å),([OII] 3727 Å)/(Hβ 4861 Å), ([OIII] 5007 Å)/(Hβ 4861 Å), ([NII] 6548Å + 6584 Å)/(Hβ 4861 Å)e ([NIII] 3869 Å)/(Hβ 4861 Å). We define as main parameters the temperature and the radius to make the modeling and observe its behavior as the temperature and the radius vary. The temperature used in the synthetic spectrum was between 1,5 × 〖10〗^5up intil7,5 × 〖10〗^5 K and the radius ranging between 1,6 up until 1,9 × 〖10〗^14 cm. |
