The isolated interacting galaxy pair ngc 5426/27 (arp 271)
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| Natura: | Artículo científico |
| Lingua: | en |
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Universidad Nacional Autónoma de México
2001
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| _version_ | 1876458767168569344 |
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| author | I. Fuentes |
| author_facet | I. Fuentes |
| contents | The isolated interacting galaxy pair ngc 5426/27 (arp 271) I. Fuentes A. Bernal H. Salo E. Laurikainen P. Amram E. Le Coarer M. Rosado D. Dultzin I. Cruz Física, Astronomía y Matemáticas GALAX NGC 5427) IES: SPIRAL GALAXIES: ISM GALAXIES: INTERACTIONS The isolated interacting galaxy pair NGC 5426/27 (Arp 271) was observedusing the scanning Fabry{Perot interferometer PUMA. The velocity eld, variouskinematical parameters and rotation curve for each galaxy were derived. We founda small bar{like structure in NGC 5426 and a severely distorted velocity eld forNGC 5427. A range of possible masses was computed for each galaxy. 2001 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101031 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.10 |
| format | Artículo científico |
| id | redalyc_57101031 |
| institution | Redalyc |
| language | en |
| publishDate | 2001 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | The isolated interacting galaxy pair ngc 5426/27 (arp 271) I. Fuentes Física, Astronomía y Matemáticas GALAX NGC 5427) IES: SPIRAL GALAXIES: ISM GALAXIES: INTERACTIONS The isolated interacting galaxy pair ngc 5426/27 (arp 271) I. Fuentes A. Bernal H. Salo E. Laurikainen P. Amram E. Le Coarer M. Rosado D. Dultzin I. Cruz Física, Astronomía y Matemáticas GALAX NGC 5427) IES: SPIRAL GALAXIES: ISM GALAXIES: INTERACTIONS The isolated interacting galaxy pair NGC 5426/27 (Arp 271) was observedusing the scanning Fabry{Perot interferometer PUMA. The velocity eld, variouskinematical parameters and rotation curve for each galaxy were derived. We founda small bar{like structure in NGC 5426 and a severely distorted velocity eld forNGC 5427. A range of possible masses was computed for each galaxy. 2001 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101031 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.10 |
| title | The isolated interacting galaxy pair ngc 5426/27 (arp 271) |
| topic | Física, Astronomía y Matemáticas GALAX NGC 5427) IES: SPIRAL GALAXIES: ISM GALAXIES: INTERACTIONS |
| url | https://www.redalyc.org/articulo.oa?id=57101031 |