Cinemática e excitação do gás em galáxias com emissão megamaser de OH
Ano de defesa: | 2018 |
---|---|
Autor(a) principal: | |
Orientador(a): | |
Banca de defesa: | , , , |
Tipo de documento: | Tese |
Tipo de acesso: | Acesso aberto |
Idioma: | por |
Instituição de defesa: |
Universidade Federal de Santa Maria
Centro de Ciências Naturais e Exatas |
Programa de Pós-Graduação: |
Programa de Pós-Graduação em Física
|
Departamento: |
Física
|
País: |
Brasil
|
Palavras-chave em Português: | |
Palavras-chave em Inglês: | |
Área do conhecimento CNPq: | |
Link de acesso: | http://repositorio.ufsm.br/handle/1/16472 |
Resumo: | We present a multiwavelength study of galaxies that host OH Megamaser emission. We used integral field unit spectroscopic data obtained with the GMOS-IFU instrument, radio data obtained with VLA and HST data for IRASF23199+0123 and IRAS03056+2034. From this data we are able to obtain information about gas dynamics and excitation in the galaxies IRASF23199+0123 and IRAS03056+2034. The main goals of this work are the identification of the central engine that ionizes the gas in these objects e propose a scenario in order to justify the OH megamaser emission. The observations of IRASF23199+0123 allow us to show that this system is formed by two interacting galaxies, in which the eastern member (IRAS23199E) presents two OH Megamaser emission hosts and the two members present extended radio emission in 3 and 20cm with the peak at the nucleus. The IFU spectroscopic data covers the inner region of IRAS23199E with 6 kpc and 2.3kpc of resolution. The flux maps constructed from this data reveal three extranuclear regions that are attributed to star forming complexes. We discovered a Seyfert 1 nucleus in IRAS23199E, due to the detection of a broad component, in the H emission-line from the BLR. Besides, the gas kinematics analysis suggests the presence of non circular motions that could be associated to the presence of outflows from the nucleus and inflows in its vicinity. The data analysis for IRAS03056+2034 does not indicate morphological evidence of interactions with other galaxies, but indicates several star forming regions along the spiral arms. The comparison between GMOS-IFU and HST observations allows the identification of a circumnuclear star forming ring. We built diagnostic diagrams that in addiction with the brightness temperature value and spectral index allow us to conclude that the gas excitation is due to not only to Starburst but also due to the presence of an AGN. The analysis of the gas kinematics suggests the presence of inflows towards to the nucleus, and coincident to the position of a patchy spiral arms that is observed in the HST image. |
id |
UFSM-20_34111a333dd0d19f9871918abc40fbff |
---|---|
oai_identifier_str |
oai:repositorio.ufsm.br:1/16472 |
network_acronym_str |
UFSM-20 |
network_name_str |
Manancial - Repositório Digital da UFSM |
repository_id_str |
|
spelling |
2019-05-08T17:53:05Z2019-05-08T17:53:05Z2018-06-29http://repositorio.ufsm.br/handle/1/16472We present a multiwavelength study of galaxies that host OH Megamaser emission. We used integral field unit spectroscopic data obtained with the GMOS-IFU instrument, radio data obtained with VLA and HST data for IRASF23199+0123 and IRAS03056+2034. From this data we are able to obtain information about gas dynamics and excitation in the galaxies IRASF23199+0123 and IRAS03056+2034. The main goals of this work are the identification of the central engine that ionizes the gas in these objects e propose a scenario in order to justify the OH megamaser emission. The observations of IRASF23199+0123 allow us to show that this system is formed by two interacting galaxies, in which the eastern member (IRAS23199E) presents two OH Megamaser emission hosts and the two members present extended radio emission in 3 and 20cm with the peak at the nucleus. The IFU spectroscopic data covers the inner region of IRAS23199E with 6 kpc and 2.3kpc of resolution. The flux maps constructed from this data reveal three extranuclear regions that are attributed to star forming complexes. We discovered a Seyfert 1 nucleus in IRAS23199E, due to the detection of a broad component, in the H emission-line from the BLR. Besides, the gas kinematics analysis suggests the presence of non circular motions that could be associated to the presence of outflows from the nucleus and inflows in its vicinity. The data analysis for IRAS03056+2034 does not indicate morphological evidence of interactions with other galaxies, but indicates several star forming regions along the spiral arms. The comparison between GMOS-IFU and HST observations allows the identification of a circumnuclear star forming ring. We built diagnostic diagrams that in addiction with the brightness temperature value and spectral index allow us to conclude that the gas excitation is due to not only to Starburst but also due to the presence of an AGN. The analysis of the gas kinematics suggests the presence of inflows towards to the nucleus, and coincident to the position of a patchy spiral arms that is observed in the HST image.Apresentamos um estudo multicomprimento de onda de galáxias com emissão megamaser de OH. São apresentados dados ópticos de espectroscopia de campo integral obtidos com o instrumento GMOS-IFU, dados rádio obtidos com o radiointerferômetro VLA e dados obtidos com o HST. A partir destes dados foi possível obter informações acerca da dinâmica e excitação do gás nas galáxias IRASF23199+0123 e IRAS03056+2034. Os objetivos que norteiam este trabalho são a identificação do mecanismo central de ionização do gás nesses objetos e propor um cenário capaz de justificar a presença de emissão de megamaser de OH. As observações da galáxia IRASF23199+0123 permitiram mostrar que este sistema é formado por duas galáxias em interação, sendo que no membro leste (IRAS23199E) foram detectadas duas fontes de emissão de megamasers de OH e os dois membros apresentam emissão rádio estendida em 3 e 20cm com pico no núcleo. Os dados ópticos de espectroscopia de campo integral cobrem uma região no interior de IRAS23199E com 6 kpc e com resolução de 2.3 kpc. Os mapas de fluxo construídos a partir desses dados evidenciaram três regiões com emissão extranuclear que foram atribuídas a complexos de formação estelar. Descobrimos a presença de um núcleo Seyfert 1, devido a detecção de uma componente larga, na linha de emissão de H proveniente da BLR. Além disso, a análise da cinemática do gás sugere a presença de movimentos não circulares que podem estar associados a presença de outflows provenientes do núcleo e inflow em sua vizinhança. A análise dos dados obtidos para IRAS03056+2034 não indica evidências morfológicas de interação com outras galáxias, mas indica diversas regiões de formação estelar ao longo dos braços espirais. A comparação dos dados obtidos com o instrumento GMOS-IFU e o HST permitiram identificar um anel de regiões de formação estelar circumnuclear. Foram construídos diagramas de diagnóstico que junto com o cálculo da temperatura de brilho e do índice espectral nos permitem concluir que a excitação do gás não se deve apenas a um Starburst, mas também a presença de um AGN. A análise da cinemática do gás sugere a presença de inflows em direção ao núcleo, coincidentes com a posição de um braço espiral descontínuo que é observado em uma imagem obtida com o HST.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPESporUniversidade Federal de Santa MariaCentro de Ciências Naturais e ExatasPrograma de Pós-Graduação em FísicaUFSMBrasilFísicaAttribution-NonCommercial-NoDerivatives 4.0 Internationalhttp://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessGaláxiasDinâmica e excitaçãoIRASF23199+0123IRAS03056+2034GalaxiesDynamics and excitationCNPQ::CIENCIAS EXATAS E DA TERRA::FISICACinemática e excitação do gás em galáxias com emissão megamaser de OHGas kinematics and excitation in OH megamaser galaxiesinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/doctoralThesisRiffel, Rogemar Andréhttp://lattes.cnpq.br/7535636807201892Sales, Dinalva Aires dehttp://lattes.cnpq.br/3928605188660824Schimoia, Jaderson da Silvahttp://lattes.cnpq.br/0849644102203962Motter, Juliana Cristinahttp://lattes.cnpq.br/8654187642185027Rembold, Sandro Barbozahttp://lattes.cnpq.br/3577967628416027Ricci, Tiago Vecchihttp://lattes.cnpq.br/5297745838613310http://lattes.cnpq.br/4675465893355969Carpes, Hekatelyne Prestes100500000006600c32f7612-cda6-434b-8a35-df1d2e93e536bfd9e323-f439-41ea-be79-59795c427c1da72b2b81-c72b-4de5-bdd2-4c7fac05fc59e5acf05e-ea66-4534-a054-b4d2dc02e5ad2a2a7ff0-0542-40d7-802c-d5f7dedc2ec79a674144-2dee-488b-be6e-f6c72ca67849e6d994b6-70f9-43c9-aa5e-ef12915b5b46reponame:Manancial - Repositório Digital da UFSMinstname:Universidade Federal de Santa Maria (UFSM)instacron:UFSMORIGINALTES_PPGFISICA_2018_CARPES_HEKATELYNE.pdfTES_PPGFISICA_2018_CARPES_HEKATELYNE.pdfTese de Doutoradoapplication/pdf5306373http://repositorio.ufsm.br/bitstream/1/16472/1/TES_PPGFISICA_2018_CARPES_HEKATELYNE.pdfcc36782c5e96da406c3fd338d4c863beMD51CC-LICENSElicense_rdflicense_rdfapplication/rdf+xml; charset=utf-8805http://repositorio.ufsm.br/bitstream/1/16472/2/license_rdf4460e5956bc1d1639be9ae6146a50347MD52LICENSElicense.txtlicense.txttext/plain; charset=utf-81956http://repositorio.ufsm.br/bitstream/1/16472/3/license.txt2f0571ecee68693bd5cd3f17c1e075dfMD53TEXTTES_PPGFISICA_2018_CARPES_HEKATELYNE.pdf.txtTES_PPGFISICA_2018_CARPES_HEKATELYNE.pdf.txtExtracted texttext/plain223646http://repositorio.ufsm.br/bitstream/1/16472/4/TES_PPGFISICA_2018_CARPES_HEKATELYNE.pdf.txt8edb68c6d87e243f0d2f4287249984baMD54THUMBNAILTES_PPGFISICA_2018_CARPES_HEKATELYNE.pdf.jpgTES_PPGFISICA_2018_CARPES_HEKATELYNE.pdf.jpgIM Thumbnailimage/jpeg3376http://repositorio.ufsm.br/bitstream/1/16472/5/TES_PPGFISICA_2018_CARPES_HEKATELYNE.pdf.jpg94f230d98f1ad378792d74cf4324e2ebMD551/164722019-05-09 03:02:27.399oai:repositorio.ufsm.br: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ório Institucionalhttp://repositorio.ufsm.br/PUBhttp://repositorio.ufsm.br/oai/requestopendoar:39132019-05-09T06:02:27Manancial - Repositório Digital da UFSM - Universidade Federal de Santa Maria (UFSM)false |
dc.title.por.fl_str_mv |
Cinemática e excitação do gás em galáxias com emissão megamaser de OH |
dc.title.alternative.eng.fl_str_mv |
Gas kinematics and excitation in OH megamaser galaxies |
title |
Cinemática e excitação do gás em galáxias com emissão megamaser de OH |
spellingShingle |
Cinemática e excitação do gás em galáxias com emissão megamaser de OH Carpes, Hekatelyne Prestes Galáxias Dinâmica e excitação IRASF23199+0123 IRAS03056+2034 Galaxies Dynamics and excitation CNPQ::CIENCIAS EXATAS E DA TERRA::FISICA |
title_short |
Cinemática e excitação do gás em galáxias com emissão megamaser de OH |
title_full |
Cinemática e excitação do gás em galáxias com emissão megamaser de OH |
title_fullStr |
Cinemática e excitação do gás em galáxias com emissão megamaser de OH |
title_full_unstemmed |
Cinemática e excitação do gás em galáxias com emissão megamaser de OH |
title_sort |
Cinemática e excitação do gás em galáxias com emissão megamaser de OH |
author |
Carpes, Hekatelyne Prestes |
author_facet |
Carpes, Hekatelyne Prestes |
author_role |
author |
dc.contributor.advisor1.fl_str_mv |
Riffel, Rogemar André |
dc.contributor.advisor1Lattes.fl_str_mv |
http://lattes.cnpq.br/7535636807201892 |
dc.contributor.advisor-co1.fl_str_mv |
Sales, Dinalva Aires de |
dc.contributor.advisor-co1Lattes.fl_str_mv |
http://lattes.cnpq.br/3928605188660824 |
dc.contributor.referee1.fl_str_mv |
Schimoia, Jaderson da Silva |
dc.contributor.referee1Lattes.fl_str_mv |
http://lattes.cnpq.br/0849644102203962 |
dc.contributor.referee2.fl_str_mv |
Motter, Juliana Cristina |
dc.contributor.referee2Lattes.fl_str_mv |
http://lattes.cnpq.br/8654187642185027 |
dc.contributor.referee3.fl_str_mv |
Rembold, Sandro Barboza |
dc.contributor.referee3Lattes.fl_str_mv |
http://lattes.cnpq.br/3577967628416027 |
dc.contributor.referee4.fl_str_mv |
Ricci, Tiago Vecchi |
dc.contributor.referee4Lattes.fl_str_mv |
http://lattes.cnpq.br/5297745838613310 |
dc.contributor.authorLattes.fl_str_mv |
http://lattes.cnpq.br/4675465893355969 |
dc.contributor.author.fl_str_mv |
Carpes, Hekatelyne Prestes |
contributor_str_mv |
Riffel, Rogemar André Sales, Dinalva Aires de Schimoia, Jaderson da Silva Motter, Juliana Cristina Rembold, Sandro Barboza Ricci, Tiago Vecchi |
dc.subject.por.fl_str_mv |
Galáxias Dinâmica e excitação IRASF23199+0123 IRAS03056+2034 |
topic |
Galáxias Dinâmica e excitação IRASF23199+0123 IRAS03056+2034 Galaxies Dynamics and excitation CNPQ::CIENCIAS EXATAS E DA TERRA::FISICA |
dc.subject.eng.fl_str_mv |
Galaxies Dynamics and excitation |
dc.subject.cnpq.fl_str_mv |
CNPQ::CIENCIAS EXATAS E DA TERRA::FISICA |
description |
We present a multiwavelength study of galaxies that host OH Megamaser emission. We used integral field unit spectroscopic data obtained with the GMOS-IFU instrument, radio data obtained with VLA and HST data for IRASF23199+0123 and IRAS03056+2034. From this data we are able to obtain information about gas dynamics and excitation in the galaxies IRASF23199+0123 and IRAS03056+2034. The main goals of this work are the identification of the central engine that ionizes the gas in these objects e propose a scenario in order to justify the OH megamaser emission. The observations of IRASF23199+0123 allow us to show that this system is formed by two interacting galaxies, in which the eastern member (IRAS23199E) presents two OH Megamaser emission hosts and the two members present extended radio emission in 3 and 20cm with the peak at the nucleus. The IFU spectroscopic data covers the inner region of IRAS23199E with 6 kpc and 2.3kpc of resolution. The flux maps constructed from this data reveal three extranuclear regions that are attributed to star forming complexes. We discovered a Seyfert 1 nucleus in IRAS23199E, due to the detection of a broad component, in the H emission-line from the BLR. Besides, the gas kinematics analysis suggests the presence of non circular motions that could be associated to the presence of outflows from the nucleus and inflows in its vicinity. The data analysis for IRAS03056+2034 does not indicate morphological evidence of interactions with other galaxies, but indicates several star forming regions along the spiral arms. The comparison between GMOS-IFU and HST observations allows the identification of a circumnuclear star forming ring. We built diagnostic diagrams that in addiction with the brightness temperature value and spectral index allow us to conclude that the gas excitation is due to not only to Starburst but also due to the presence of an AGN. The analysis of the gas kinematics suggests the presence of inflows towards to the nucleus, and coincident to the position of a patchy spiral arms that is observed in the HST image. |
publishDate |
2018 |
dc.date.issued.fl_str_mv |
2018-06-29 |
dc.date.accessioned.fl_str_mv |
2019-05-08T17:53:05Z |
dc.date.available.fl_str_mv |
2019-05-08T17:53:05Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/doctoralThesis |
format |
doctoralThesis |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://repositorio.ufsm.br/handle/1/16472 |
url |
http://repositorio.ufsm.br/handle/1/16472 |
dc.language.iso.fl_str_mv |
por |
language |
por |
dc.relation.cnpq.fl_str_mv |
100500000006 |
dc.relation.confidence.fl_str_mv |
600 |
dc.relation.authority.fl_str_mv |
c32f7612-cda6-434b-8a35-df1d2e93e536 bfd9e323-f439-41ea-be79-59795c427c1d a72b2b81-c72b-4de5-bdd2-4c7fac05fc59 e5acf05e-ea66-4534-a054-b4d2dc02e5ad 2a2a7ff0-0542-40d7-802c-d5f7dedc2ec7 9a674144-2dee-488b-be6e-f6c72ca67849 e6d994b6-70f9-43c9-aa5e-ef12915b5b46 |
dc.rights.driver.fl_str_mv |
Attribution-NonCommercial-NoDerivatives 4.0 International http://creativecommons.org/licenses/by-nc-nd/4.0/ info:eu-repo/semantics/openAccess |
rights_invalid_str_mv |
Attribution-NonCommercial-NoDerivatives 4.0 International http://creativecommons.org/licenses/by-nc-nd/4.0/ |
eu_rights_str_mv |
openAccess |
dc.publisher.none.fl_str_mv |
Universidade Federal de Santa Maria Centro de Ciências Naturais e Exatas |
dc.publisher.program.fl_str_mv |
Programa de Pós-Graduação em Física |
dc.publisher.initials.fl_str_mv |
UFSM |
dc.publisher.country.fl_str_mv |
Brasil |
dc.publisher.department.fl_str_mv |
Física |
publisher.none.fl_str_mv |
Universidade Federal de Santa Maria Centro de Ciências Naturais e Exatas |
dc.source.none.fl_str_mv |
reponame:Manancial - Repositório Digital da UFSM instname:Universidade Federal de Santa Maria (UFSM) instacron:UFSM |
instname_str |
Universidade Federal de Santa Maria (UFSM) |
instacron_str |
UFSM |
institution |
UFSM |
reponame_str |
Manancial - Repositório Digital da UFSM |
collection |
Manancial - Repositório Digital da UFSM |
bitstream.url.fl_str_mv |
http://repositorio.ufsm.br/bitstream/1/16472/1/TES_PPGFISICA_2018_CARPES_HEKATELYNE.pdf http://repositorio.ufsm.br/bitstream/1/16472/2/license_rdf http://repositorio.ufsm.br/bitstream/1/16472/3/license.txt http://repositorio.ufsm.br/bitstream/1/16472/4/TES_PPGFISICA_2018_CARPES_HEKATELYNE.pdf.txt http://repositorio.ufsm.br/bitstream/1/16472/5/TES_PPGFISICA_2018_CARPES_HEKATELYNE.pdf.jpg |
bitstream.checksum.fl_str_mv |
cc36782c5e96da406c3fd338d4c863be 4460e5956bc1d1639be9ae6146a50347 2f0571ecee68693bd5cd3f17c1e075df 8edb68c6d87e243f0d2f4287249984ba 94f230d98f1ad378792d74cf4324e2eb |
bitstream.checksumAlgorithm.fl_str_mv |
MD5 MD5 MD5 MD5 MD5 |
repository.name.fl_str_mv |
Manancial - Repositório Digital da UFSM - Universidade Federal de Santa Maria (UFSM) |
repository.mail.fl_str_mv |
|
_version_ |
1794524332074991616 |