The relation between the Black hole mass and the Bulge mass for low redshift AGNs. Part I: Ground-based observations

Using the bulge data from AGN image decomposition with ground-based observations, we calculate the ratios of the central supermassive black hole mass(SMBH) to the Bulge mass (_Mbh/_Mbulge$M_{\text{bh}}/M_{\text{bulge}}$) in a sample of X-ray selected AGNs, including 15 Narrow-line Seyfert 1 galaxies (NLS1s) and 18 broad-line Seyfert 1 galaxies (BLS1s). We found that the mean value of log(_Mbh/_Mbulge)$\log (M_{\text{bh}}/M_{\text{bulge}})$ is -3.81±0.11$-3.81\pm 0.11$ for 15 NLS1s, and -2.91±0.13$-2.91\pm 0.13$ for 18 BLS1s, showing the lower _Mbh/_Mbulge$M_{\text{bh}}/M_{\text{bulge}}$ in NLS1s relative to BLS1s. The calculation shows that the Bulge mass from the host image decomposition in NLS1s is statistically smaller than that from Hubble-type correction method, and a linear mass relation is suggested for NLS1s and a nonlinear mass relation for BLS1s. The studying of host galaxies with ground-based observations strongly limited by the atmospheric seeing. We need to do the decomposition of host images for NLS1s with Hubble Space Telescope observation in the future.     

鼓包对双立尾/三角翼立尾抖振的影响

为了研究鼓包对立尾抖振的影响,在北航的水槽和风洞中进行了在机翼头部放置了鼓包的75°后掠双立尾-三角翼的立尾抖振实验,采用了流动显示、立尾表面动态压力测量、激光测立尾顶部加速度的实验来检验鼓包对立尾抖振减缓的效果。流动显示的实验结果表明三角翼机翼头部加上鼓包后,前缘涡涡核会发生弯曲和扭转,这在一定程度上减弱了前缘涡。激光测立尾顶部加速度实验的结果表明,在25°到48°这段立尾抖振比较显著的迎角范围内,A1立尾位置的立尾抖振强度曲线比无鼓包的曲线数值上有明显的减小,抖振得到一定的改善。立尾表面动态压力的脉动强度也有明显的减小,前缘涡涡核的弯曲和扭转起到了减缓立尾抖振的作用。