A BAYESIAN MONTE CARLO ANALYSIS OF THE M-σ RELATION

被引:10
|
作者
Morabito, Leah K. [1 ]
Dai, Xinyu [1 ]
机构
[1] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA
来源
ASTROPHYSICAL JOURNAL | 2012年 / 757卷 / 02期
关键词
black hole physics; galaxies: fundamental parameters; galaxies: general; methods: statistical; SUPERMASSIVE BLACK-HOLES; VELOCITY DISPERSION CORRELATION; ACTIVE GALACTIC NUCLEI; LINE QUASAR FRACTION; M-BH; GALAXY FORMATION; COSMOLOGICAL SIMULATIONS; HOST GALAXIES; FEEDBACK; MASS;
D O I
10.1088/0004-637X/757/2/172
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an analysis of selection biases in the M-bh-sigma relation using Monte Carlo simulations including the sphere of influence resolution selection bias and a selection bias in the velocity dispersion distribution. We find that the sphere of influence selection bias has a significant effect on the measured slope of the M-bh-sigma relation, modeled as beta(intrinsic) = -4.69+2.22 beta(measured), where the measured slope is shallower than the model slope in the parameter range of beta > 4, with larger corrections for steeper model slopes. Therefore, when the sphere of influence is used as a criterion to exclude unreliable measurements, it also introduces a selection bias that needs to be modeled to restore the intrinsic slope of the relation. We find that the selection effect due to the velocity dispersion distribution of the sample, which might not follow the overall distribution of the population, is not important for slopes of beta similar to 4-6 of a logarithmically linear M-bh-sigma relation, which could impact some studies that measure low (e.g., beta < 4) slopes. Combining the selection biases in velocity dispersions and the sphere of influence cut, we find that the uncertainty of the slope is larger than the value without modeling these effects and estimate an intrinsic slope of beta = 5.28(-055)(+0.84).
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页数:9
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