Circumnuclear structures in the interacting Seyfert galaxy NGC 1241 : kinematics and optical/infrared morphology
Autor(a) principal: | |
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Data de Publicação: | 2003 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/108909 |
Resumo: | We studied the spiral pattern in the inner 6".5 (1" = 257 pc) central regions of the interacting active nucleus galaxy NGC 1241 using Gemini North Telescope high-resolution Ks- and J-band images and Hubble Space Telescope (HST) Paα and H- and (V+R)-band images with high resolution in the range from ~0".1 to ~0".3 along with intermediate to large-scale spectroscopy using the Multifunction Spectrograph at the Córdoba Observatory in Argentina. Our analysis of Paα emission images revealed a faint two-armed leading spiral pattern ending in the 5".6 x 3".4 clumpy ring discovered by Böker and coworkers, harboring a 1".6 long barlike structure almost perpendicular to the large-scale bar of NGC 1241. When we applied two-dimensional Fourier analysis at circumnuclear scales, we found that a two-arm trailing mode was dominant in Ks- and J-band images while the (V+R)-band images showed more complex structural features with a strong onearmed trailing mode. One-dimensional Fourier analysis showed a corotation (CR) located outward from the edge of the Paα bar. Our kinematics data gave an angular speed ΩCN of 350±50 km s-ˡ kpc-ˡ for the trailing mode pattern. The rotation curve showed that the circumnuclear ring is located just inside the large-scale pattern inner Lindblad resonance (ILR), which has a radius of about ~1 kpc. We also found, within the uncertainties present in such measurements, that the outer Lindblad resonance (OLR) of the circumnuclear pattern is coincident with the large-scale pattern ILR, indicating a possible connection between circumnuclear and global dynamics. Nevertheless, the estimated high molecular gas fraction (≥13%) and the inner pattern high angular speed at the central region of NGC 1241 point to a nuclear bar formation via self-gravitational instability. |
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Díaz, Rubén JoaquínDottori, Horacio AlbertoVera Villamizar, NelsonCarranza, Gustavo Jose2015-01-14T02:15:54Z20030004-637Xhttp://hdl.handle.net/10183/108909000397180We studied the spiral pattern in the inner 6".5 (1" = 257 pc) central regions of the interacting active nucleus galaxy NGC 1241 using Gemini North Telescope high-resolution Ks- and J-band images and Hubble Space Telescope (HST) Paα and H- and (V+R)-band images with high resolution in the range from ~0".1 to ~0".3 along with intermediate to large-scale spectroscopy using the Multifunction Spectrograph at the Córdoba Observatory in Argentina. Our analysis of Paα emission images revealed a faint two-armed leading spiral pattern ending in the 5".6 x 3".4 clumpy ring discovered by Böker and coworkers, harboring a 1".6 long barlike structure almost perpendicular to the large-scale bar of NGC 1241. When we applied two-dimensional Fourier analysis at circumnuclear scales, we found that a two-arm trailing mode was dominant in Ks- and J-band images while the (V+R)-band images showed more complex structural features with a strong onearmed trailing mode. One-dimensional Fourier analysis showed a corotation (CR) located outward from the edge of the Paα bar. Our kinematics data gave an angular speed ΩCN of 350±50 km s-ˡ kpc-ˡ for the trailing mode pattern. The rotation curve showed that the circumnuclear ring is located just inside the large-scale pattern inner Lindblad resonance (ILR), which has a radius of about ~1 kpc. We also found, within the uncertainties present in such measurements, that the outer Lindblad resonance (OLR) of the circumnuclear pattern is coincident with the large-scale pattern ILR, indicating a possible connection between circumnuclear and global dynamics. Nevertheless, the estimated high molecular gas fraction (≥13%) and the inner pattern high angular speed at the central region of NGC 1241 point to a nuclear bar formation via self-gravitational instability.application/pdfengThe astrophysical journal. Chicago. Vol. 597, no. 2 pt. 1 (Nov. 2003), p. 860-869Fotometria astronômicaEspectros astronômicosAnálise de FourierNucleo galaticoFontes de infravermelhoGalaxias seyfertGalaxies: activeGalaxies: individual (NGC 1241)Galaxies: kinematics and dynamicsGalaxies: spiralGalaxies: structureMethods: numericalTechniques: spectroscopicCircumnuclear structures in the interacting Seyfert galaxy NGC 1241 : kinematics and optical/infrared morphologyEstrangeiroinfo: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:UFRGSORIGINAL000397180.pdf000397180.pdfTexto completo (inglês)application/pdf771310http://www.lume.ufrgs.br/bitstream/10183/108909/1/000397180.pdfa15638e324cfaf989690f0ac5569fa2fMD51TEXT000397180.pdf.txt000397180.pdf.txtExtracted Texttext/plain44832http://www.lume.ufrgs.br/bitstream/10183/108909/2/000397180.pdf.txta835d04c3b4f99a1f8c8bccf2006a0d5MD52THUMBNAIL000397180.pdf.jpg000397180.pdf.jpgGenerated Thumbnailimage/jpeg1788http://www.lume.ufrgs.br/bitstream/10183/108909/3/000397180.pdf.jpg5b62a7586dfe7c838e659272d762209fMD5310183/1089092022-02-22 05:02:03.157627oai:www.lume.ufrgs.br:10183/108909Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2022-02-22T08:02:03Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Circumnuclear structures in the interacting Seyfert galaxy NGC 1241 : kinematics and optical/infrared morphology |
title |
Circumnuclear structures in the interacting Seyfert galaxy NGC 1241 : kinematics and optical/infrared morphology |
spellingShingle |
Circumnuclear structures in the interacting Seyfert galaxy NGC 1241 : kinematics and optical/infrared morphology Díaz, Rubén Joaquín Fotometria astronômica Espectros astronômicos Análise de Fourier Nucleo galatico Fontes de infravermelho Galaxias seyfert Galaxies: active Galaxies: individual (NGC 1241) Galaxies: kinematics and dynamics Galaxies: spiral Galaxies: structure Methods: numerical Techniques: spectroscopic |
title_short |
Circumnuclear structures in the interacting Seyfert galaxy NGC 1241 : kinematics and optical/infrared morphology |
title_full |
Circumnuclear structures in the interacting Seyfert galaxy NGC 1241 : kinematics and optical/infrared morphology |
title_fullStr |
Circumnuclear structures in the interacting Seyfert galaxy NGC 1241 : kinematics and optical/infrared morphology |
title_full_unstemmed |
Circumnuclear structures in the interacting Seyfert galaxy NGC 1241 : kinematics and optical/infrared morphology |
title_sort |
Circumnuclear structures in the interacting Seyfert galaxy NGC 1241 : kinematics and optical/infrared morphology |
author |
Díaz, Rubén Joaquín |
author_facet |
Díaz, Rubén Joaquín Dottori, Horacio Alberto Vera Villamizar, Nelson Carranza, Gustavo Jose |
author_role |
author |
author2 |
Dottori, Horacio Alberto Vera Villamizar, Nelson Carranza, Gustavo Jose |
author2_role |
author author author |
dc.contributor.author.fl_str_mv |
Díaz, Rubén Joaquín Dottori, Horacio Alberto Vera Villamizar, Nelson Carranza, Gustavo Jose |
dc.subject.por.fl_str_mv |
Fotometria astronômica Espectros astronômicos Análise de Fourier Nucleo galatico Fontes de infravermelho Galaxias seyfert |
topic |
Fotometria astronômica Espectros astronômicos Análise de Fourier Nucleo galatico Fontes de infravermelho Galaxias seyfert Galaxies: active Galaxies: individual (NGC 1241) Galaxies: kinematics and dynamics Galaxies: spiral Galaxies: structure Methods: numerical Techniques: spectroscopic |
dc.subject.eng.fl_str_mv |
Galaxies: active Galaxies: individual (NGC 1241) Galaxies: kinematics and dynamics Galaxies: spiral Galaxies: structure Methods: numerical Techniques: spectroscopic |
description |
We studied the spiral pattern in the inner 6".5 (1" = 257 pc) central regions of the interacting active nucleus galaxy NGC 1241 using Gemini North Telescope high-resolution Ks- and J-band images and Hubble Space Telescope (HST) Paα and H- and (V+R)-band images with high resolution in the range from ~0".1 to ~0".3 along with intermediate to large-scale spectroscopy using the Multifunction Spectrograph at the Córdoba Observatory in Argentina. Our analysis of Paα emission images revealed a faint two-armed leading spiral pattern ending in the 5".6 x 3".4 clumpy ring discovered by Böker and coworkers, harboring a 1".6 long barlike structure almost perpendicular to the large-scale bar of NGC 1241. When we applied two-dimensional Fourier analysis at circumnuclear scales, we found that a two-arm trailing mode was dominant in Ks- and J-band images while the (V+R)-band images showed more complex structural features with a strong onearmed trailing mode. One-dimensional Fourier analysis showed a corotation (CR) located outward from the edge of the Paα bar. Our kinematics data gave an angular speed ΩCN of 350±50 km s-ˡ kpc-ˡ for the trailing mode pattern. The rotation curve showed that the circumnuclear ring is located just inside the large-scale pattern inner Lindblad resonance (ILR), which has a radius of about ~1 kpc. We also found, within the uncertainties present in such measurements, that the outer Lindblad resonance (OLR) of the circumnuclear pattern is coincident with the large-scale pattern ILR, indicating a possible connection between circumnuclear and global dynamics. Nevertheless, the estimated high molecular gas fraction (≥13%) and the inner pattern high angular speed at the central region of NGC 1241 point to a nuclear bar formation via self-gravitational instability. |
publishDate |
2003 |
dc.date.issued.fl_str_mv |
2003 |
dc.date.accessioned.fl_str_mv |
2015-01-14T02:15:54Z |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
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article |
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0004-637X |
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000397180 |
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http://hdl.handle.net/10183/108909 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
The astrophysical journal. Chicago. Vol. 597, no. 2 pt. 1 (Nov. 2003), p. 860-869 |
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