Thick disk and pseudobulge formation in a clump cluster
Bulges in spiral galaxies have been supposed to be classified into two types: classical bulges or pseudobulges. Classical bulges are thought to form by galactic merger with bursty star formation, whereas pseudobulges are suggested to form by secular evolution. Noguchi (1998,199) suggested another bu...
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| Autor principal: | |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
EDP Sciences
2012-02-01
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| coleção: | EPJ Web of Conferences |
| Acesso em linha: | http://dx.doi.org/10.1051/epjconf/20121904005 |
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