Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Orjales, J. M. Cao"'
Autor:
Khan-Ali, A., Carrera, F. J., Page, M. J., Stevens, J. A., Mateos, S., Symeonidis, M., Orjales, J. M. Cao
We have assembled a sample of 5 X-ray-absorbed and submm-luminous type 1 QSOs at $z \sim 2$ which are simultaneously growing their central black holes through accretion and forming stars copiously. We present here the analysis of their rest-frame UV
Externí odkaz:
http://arxiv.org/abs/1501.02095
Autor:
Khan-Ali, A., Carrera, F. J., Page, M. J., Stevens, J. A., Mateos, S., Symeonidis, M., Orjales, J. M. Cao
We present a detailed study of a X -ray selected sample of 5 submillimeter bright QSOs at $z\sim2$, where the highest rates of star formation (SF) and further growth of black holes (BH) occur. Therefore, this sample is a great laboratory to investiga
Externí odkaz:
http://arxiv.org/abs/1412.1250
We have assembled a sample of 5 X-ray and submm-luminous z~2 QSOs which are therefore both growing their central black holes through accretion and forming stars copiously at a critical epoch. Hence, they are good laboratories to investigate the co-ev
Externí odkaz:
http://arxiv.org/abs/1302.2844
Autor:
Orjales, J. M. Cao, Stevens, J. A., Jarvis, M. J., Smith, D. J. B., Hardcastle, M. J., Auld, R., Baes, M., Cava, A., Clements, D. L., Cooray, A., Coppin, K., Dariush, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Hopwood, R., Hoyos, C., Ibar, E., Ivison, R. J., Maddox, S., Page, M. J., Valiante, E.
We have used data from the Herschel-ATLAS at 250, 350 and 500 \mu m to determine the far-infrared (FIR) properties of 50 Broad Absorption Line Quasars (BAL QSOs). Our sample contains 49 high-ionization BAL QSOs (HiBALs) and 1 low-ionization BAL QSO (
Externí odkaz:
http://arxiv.org/abs/1209.0670
Autor:
Khan-Ali, A., Carrera, F. J., Page, M. J., Stevens, J. A., Mateos, S., Symeonidis, M., Orjales, J. M. Cao
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Mar2015, Vol. 448 Issue 1, p75-89, 15p