| タイトル | The spectrum of the halo surrounding the quasar PHL 1070 |
| 著者（英） | Morton, D. C.; Green, R. F.; Williams, T. B. |
| 著者所属（英） | Hale Observatories|Princeton Univ. Observatory |
| 発行日 | 1978-01-15 |
| 言語 | eng |
| 内容記述 | The quasar PHL 1070 and its surrounding halo of light have been observed with the Palomar multichannel spectrophotometer using circular and annular apertures. The central quasar has a magnitude of 16.6 and an emission-line redshift of 0.076 + or - 0.002. The halo light has a magnitude of 19.0 and a possible absorption-line system with an absorption redshift of 0.067 + or - 0.008. The magnitude, possible absorption lines, and probable spectral energy distribution of the halo are consistent with those of a normal galaxy at the redshift of the quasar. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 78A22280 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/433964 |
