Red Parkes quasars: Evidence for soft X-ray absorption

被引:8
|
作者
Masci, FJ [1 ]
Drinkwater, MJ
Webster, RL
机构
[1] Univ Melbourne, Sch Phys, Astrophys Grp, Melbourne, Vic 3052, Australia
[2] Univ New S Wales, Dept Astrophys & Opt, Sch Phys, Sydney, NSW 2052, Australia
来源
ASTROPHYSICAL JOURNAL | 1999年 / 510卷 / 02期
关键词
dust; extinction; ISM : general; quasars : general; X-rays : ISM;
D O I
10.1086/306611
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Parkes Half-Jansky Flat-Spectrum Sample contains a large number of sources with unusually red optical-to-near-infrared (NIR) continua. If this is to be interpreted as extinction by dust in the line of sight, then associated material might also give rise to absorption in the soft X-ray regime. This hypothesis is tested using broadband (0.1-2.4 keV) data from the ROSAT All-Sky Survey. Significant (>3 sigma confidence level) correlations between the optical (and NIR)-to-soft X-ray continuum slope and optical extinction are found in the data, consistent with absorption by material with metallicity and a range in the gas-to-dust ratio as observed in the local ISM. Under this simple model, the soft X-rays are absorbed at a level consistent with the range of extinctions (0 < A(V) < 6 mag) implied by the observed optical reddening. Excess X-ray absorption by warm (ionized) gas, (i.e., a warm absorber) is not required by the data.
引用
收藏
页码:703 / 709
页数:7
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