论文标题
TXS 2226-184核心的黑洞质量距离比的一般相对论估计
A general relativistic estimation of the black hole mass-to-distance ratio at the core of TXS 2226-184
论文作者
论文摘要
在这项工作中，我们利用一种一般的相对论方法来估计质量比= 3.54^{+0.2} _ { - 0.2} x 10^4 m_ {sun}/mpc，在其右浪费核心的核心核心的核心核心的黑洞和右浪费均与访问范围内的核心核心均托有的核心范围（均可及其RECESTION）的范围（VEL）。 星系。我们的统计拟合是基于水层发出的光子及其轨道位置的频移，当时在活性银河核的积聚盘内圆形旋转时。通过考虑到先前报道的与银河系的距离，我们将黑洞质量拟合的结果与基于质量劳度相关性的估计值进行了比较。 We find that the black hole mass at the core of TXS 2226-184 obtained with the aid of the statistical fit using the general relativistic method, M = 3.67 ^{+0.2}_{-0.2} X 10^6 M_{sun}, is approximately 0.6 times the black hole mass, M_{BH} = 6.24^{+3.6}_{-2.3} X 10^6 m_ {sun}，以质量 - 露光性相关性计算。
In this work we make use of a general relativistic method to estimate the mass-to-distance ratio M/D = 3.54^{+0.2}_{-0.2} X 10^4 M_{sun}/Mpc of the black hole hosted at the core of the active galactic nucleus of TXS 2226-184, along with its Right Ascension offset and the recession redshift (velocity) of the galaxy. Our statistical fit is based on the frequency shift of photons emitted by water masers and their orbital positions when circularly revolving around the black hole center within the accretion disk of the active galactic nucleus. By taking into account a previously reported distance to the galaxy, we compare the result of the black hole mass fit to an estimate based on a mass-luminosity correlation. We find that the black hole mass at the core of TXS 2226-184 obtained with the aid of the statistical fit using the general relativistic method, M = 3.67 ^{+0.2}_{-0.2} X 10^6 M_{sun}, is approximately 0.6 times the black hole mass, M_{BH} = 6.24^{+3.6}_{-2.3} X 10^6 M_{sun}, computed with the mass-luminosity correlation.
