Building blocks of the most luminous galaxies
Nearby luminous galaxies serve as templates to gain insight into the building blocks of the most luminous galaxies in the distant universe. In this conference I have shown that the most luminous galaxies in the Local Universe are mergers of evolved gas-rich galaxies that radiate the bulk of their en...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
2002
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 02951caa a22004457a 4500 | ||
|---|---|---|---|
| 001 | PAPER-20233 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518205137.0 | ||
| 008 | 190411s2002 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-0141458800 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Mirabel, I.F. | |
| 245 | 1 | 0 | |a Building blocks of the most luminous galaxies |
| 260 | |c 2002 | ||
| 270 | 1 | 0 | |m Mirabel, I.F.; CEA/DSM/DAPNIA, Service d 'Astrophysique, 91191 Gif/Yvette, France |
| 506 | |2 openaire |e Política editorial | ||
| 504 | |a Kim, D.C., (1995) The IRAS 1 Jy Survey of Ultraluminous Infrared Galaxies, , PhD thesis, Univ. Hawaii | ||
| 504 | |a Le Floc'h, E., Mirabel, I.F., Laurent, O., (1999), in preparation; Melnick, J., Mirabel, I.F., (1990) A&A, 231, pp. L19 | ||
| 504 | |a Mirabel, I.F., Lutz, D., Maza, J., (1991) A&A, 243, p. 367 | ||
| 504 | |a Sanders, D.B., Mirabel, I.F., (1996) ARAA, 34, p. 749 | ||
| 504 | |a Sanders, D.B., Soifer, B.T., Flias, J.H., (1988) ApJ, 325, p. 74 | ||
| 504 | |a Sanders, D.B., Soifer, B.T., Elias, J.H., Neugebauer, G., Matthews, K., (1988) ApJ, 328, pp. L35 | ||
| 504 | |a Soifer, B.T., Sanders, D.B., Madore, B.F., Neugebuer, G., (1987) ApJ, 320, p. 238 | ||
| 504 | |a Soifer, B.T., Neugebauer, G., (1991) AJ, 101, p. 354 | ||
| 520 | 3 | |a Nearby luminous galaxies serve as templates to gain insight into the building blocks of the most luminous galaxies in the distant universe. In this conference I have shown that the most luminous galaxies in the Local Universe are mergers of evolved gas-rich galaxies that radiate the bulk of their energy in the mid and far-infrared. The most important implication for future studies on the formation of galaxies at early cosmological timescales is that they will appear as luminous sub-millimeter sources. |l eng | |
| 593 | |a CEA/DSM/DAPNIA, Service d 'Astrophysique, 91191 Gif/Yvette, France | ||
| 593 | |a IAFE/CONICET, Ciudad Universitaria, 1428 Buenos Aires, Argentina | ||
| 690 | 1 | 0 | |a GALAXIES: DWARF |
| 690 | 1 | 0 | |a GALAXIES: NUCLEI |
| 690 | 1 | 0 | |a GALAXIES: STARBURST |
| 690 | 1 | 0 | |a INFRARED: GALAXIES |
| 773 | 0 | |d 2002 |g v. 281 |h pp. 375-378 |k n. 1-2 |p Astrophys. Space Sci. |x 0004640X |w (AR-BaUEN)CENRE-3855 |t Astrophysics and Space Science | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-0141458800&doi=10.1023%2fA%3a1019517131594&partnerID=40&md5=15041ca128d13b7a9e7419520abc538a |y Registro en Scopus |
| 856 | 4 | 0 | |u https://doi.org/10.1023/A:1019517131594 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_0004640X_v281_n1-2_p375_Mirabel |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004640X_v281_n1-2_p375_Mirabel |y Registro en la Biblioteca Digital |
| 961 | |a paper_0004640X_v281_n1-2_p375_Mirabel |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/article |a info:ar-repo/semantics/artículo |b info:eu-repo/semantics/publishedVersion | ||
| 963 | |a VARI | ||
| 999 | |c 81186 | ||