The MBH-M relation for X-ray-obscured, red QSOs at 1.2 < z < 2.6
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2014-09, Vol.443 (3), p.2077-2091 |
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| container_end_page | 2091 |
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| container_issue | 3 |
| container_start_page | 2077 |
| container_title | Monthly notices of the Royal Astronomical Society |
| container_volume | 443 |
| creator | Bongiorno, A. Maiolino, R. Brusa, M. Marconi, A. Piconcelli, E. Lamastra, A. Cano-Díaz, M. Schulze, A. Magnelli, B. Vignali, C. Fiore, F. Menci, N. Cresci, G. La Franca, F. Merloni, A. |
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| doi_str_mv | 10.1093/mnras/stu1248 |
| format | Article |
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| fulltext | fulltext |
| identifier | ISSN: 0035-8711 |
| ispartof | Monthly notices of the Royal Astronomical Society, 2014-09, Vol.443 (3), p.2077-2091 |
| issn | 0035-8711 1365-2966 |
| language | eng |
| recordid | cdi_crossref_primary_10_1093_mnras_stu1248 |
| source | Oxford Journals Open Access Collection |
| title | The MBH-M relation for X-ray-obscured, red QSOs at 1.2 < z < 2.6 |
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