The Supermassive Black Hole in NGC 4258 Distance, Mass and Measuring the Black Hole Bulge Mass Ratio

The Supermassive Black Hole in NGC 4258 Distance, Mass and Measuring the Black Hole Bulge Mass Ratio

The Supermassive Black Hole in NGC 4258 Distance, Mass and measuring the black hole bulge mass ratio Group 1: Rubén Herrero-Illana Joachim Janz Sara Lindgren Paulo Santos NGC 4258 (M106) 12:18:57.5 +47:18:14 7.44 Mpc H2O megamaser Observations VLBA 20m NOT Aim: Physical properties by using the water MASER Megamasers Megamasers Megamasers Megamasers Megamasers Megamasers Megamasers Very Long Baseline Array Observations at 22 GHz Bandwidth: 16 MHz Resolution: 31.25 KHz Redshifted + Systemic masers VLBA Data Reduction Calibration: AIPS + ParselTongue Imaging and deconvolution: CASA VLBA Data Cubes Click to edit Master text styles Second level ● Third level ● Fourth level ● Fifth level Redshifte d VLBA Data Cubes Click to edit Master text styles Second level ● Third level ● Fourth level ● Fifth level Systemic VLBA Results Click to edit Master text styles Second level ● Third level ● Fourth level ● Fifth level So far… so good So far… so good So far… so good 20-m single dish Gaussian fit 15.2 ± 0.1 km/s per year 5.2 ± 0.1 km/s per year Cross-correlation 5 km/s per year 1.6 1.4 1.2 1 ] y J [ y t 0.8 i s n e t n I 0.6 0.4 0.2 0 500 495 490 485 480 475 470 465 460 velocity [km/s] Result - VLBA and 20-m telescope Velocity: 956.6 ± 99.3 km/s Angular distance: -4.53 ± 2.18 milli-arcsec Distance to the NGC4258: 8.51 ± 5.93 Mpc Acceleration: 5.2 ± 0.1 km/s per year Radius of the inner region: 0.19 ± 0.09 pc Mass inside the inner radius: 3.98 ± 1.04 *107 M Nordic Optical Telescope B, R, J, H and K band M-to-L relation 12 Observation Sersic Exponential Model 13 2MASS 14 2 c 15 e s c r a / g a 16 m 17 18 19 0 20 40 60 80 100 arcsec compare with 2MASS compare sky frames and sky Disk – Exponential fit Bulge Sérsic fit– obtain the luminosity in in bulgethe the K-band Integral of profile to Integral of profile GALFIT software Calibrate with stars in the Bulge-disk decomposition Compare with M-to-L relation from previous literature: Bell and de Jong, ApJ, 2001 • Mass-to-light ratio of ~1.3 12.5 Marconi and Hunt 2003 12 Marconi and 11.5 11 K 10.5 M 10 9.5 9 8.5 -28 -27 -26 -25 -24 -23 -22 -21 -20 -19 log(BM) LK vs log(Mbulge) from literature: literature: vs log(Mbulge)LK from Hunt, ApJ, 2003 10 9.5 B-R M. and H. Marconi and Hunt 2003 9 8.5 ) H B M 8 ( g o l 7.5 7 6.5 6 8.5 9 9.5 10 10.5 11 11.5 12 12.5 log(bMulg)e 0.6*1010 M 0.6*1010 M 0.3*1010 Black hole to bulge mass relation Bulge mass Summary This project Literature Velocity 956.6 ± 99.3 km/s 1080 ± 2 km/s Angular distance -4.53 ± 2.18 milli- -4.4 milli-arcsec arcsec Acceleration 5.2 ± 0.1 km/s per 10 km/s per year year Radius of the inner 0.19 ± 0.09 pc 0.13 pc region Distance to NGC4258 8.51 ± 5.93 Mpc 7.44 Mpc Mass inside the inner 3.98 ± 1.04 *107 M 3.6*107 M radius Bulge mass 0.3-0.6 *1010 M 1.1 *1010 M.

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