WISDOM Project - III. Molecular gas measurement of the supermassive black hole mass in the barred lenticular galaxy NGC4429

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 473:3 (2018) 3818-3834

Authors:

Timothy A Davis, Martin Bureau, Kyoko Onishi, Freeke van de Voort, Michele Cappellari, Satoru Iguchi, Lijie Liu, Eve V North, Marc Sarzi, Mark D Smith

SNe 2013K and 2013am: observed and physical properties of two slow, normal Type IIP events

(2017)

Authors:

L Tomasella, E Cappellaro, ML Pumo, A Jerkstrand, S Benetti, N Elias-Rosa, M Fraser, C Inserra, A Pastorello, M Turatto, JP Anderson, L Galbany, CP Gutierrez, E Kankare, G Pignata, G Terreran, S Valenti, C Barbarino, FE Bauer, MT Botticella, TW Chen, A Gal-Yam, A Harutyunyan, DA Howell, K Maguire, A Morales Garoffolo, P Ochner, SJ Smartt, S Schulze, DR Young, L Zampieri

The SAMI Galaxy Survey: global stellar populations on the size-mass plane

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 472:3 (2017) 2833-2855

Authors:

N Scott, S Brough, SM Croom, RL Davies, J van de Sande, JT Allen, J Bland-Hawthorn, JJ Bryant, L Cortese, F D'Eugenio, C Federrath, I Ferreras, M Goodwin, B Groves, I Konstantopoulos, JS Lawrence, AM Medling, AJ Moffett, MS Owers, S Richards, ASG Robotham, C Tonini, SK Yi

SDSS-IV MaNGA-resolved Star Formation and Molecular Gas Properties of Green Valley Galaxies: A First Look with ALMA and MaNGA

The Astrophysical Journal American Astronomical Society 851:1 (2017) 18

Authors:

Lihwai Lin, Francesco Belfiore, Hsi-An Pan, MS Bothwell, Pei-Ying Hsieh, Shan Huang, Ting Xiao, Sebastián F Sánchez, Bau-Ching Hsieh, Karen Masters, S Ramya, Jing-Hua Lin, Chin-Hao Hsu, Cheng Li, Roberto Maiolino, Kevin Bundy, Dmitry Bizyaev, Niv Drory, Héctor Ibarra-Medel, Ivan Lacerna, Tim Haines, Rebecca Smethurst, David V Stark, Daniel Thomas

A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni

Science American Association for the Advancement of Science 358:6368 (2017)

Authors:

Y Dallilar, SS Eikenberry, A Garner, RD Stelter, A Gottlieb, P Gandhi, P Casella, VS Dhillon, TR Marsh, SP Littlefair, L Hardy, Robert Fender, Kunal Mooley, DJ Walton, F Fuerst, M Bachetti, AJ Castro-Tirado, M Charcos, ML Edwards, NM Lasso-Cabrera, A Marin-Franch, K Ackley, JG Bennett, AJ Cenarro, B Chinn, HV Donoso, R Frommeyer, K Hanna, J Julian, P Miller, S Mullin, CH Murphey, C Packham, F Varosi, C Vega, C Warner, AN Ramaprakash, M Burse, S Punnadi, P Chordia, A Gerarts, H De Paz Martín, MM Calero, R Scarpa, SF Acosta, B Siegel, FF Pérez

Abstract:

Observations of binary stars containing an accreting black hole or neutron star often show x-ray emission extending to high energies (>10 kilo--electron volts), which is ascribed to an accretion disk corona of energetic particles akin to those seen in the solar corona. Despite their ubiquity, the physical conditions in accretion disk coronae remain poorly constrained. Using simultaneous infrared, optical, x-ray, and radio observations of the Galactic black hole system V404 Cygni, showing a rapid synchrotron cooling event in its 2015 outburst, we present a precise 461 ± 12 gauss magnetic field measurement in the corona. This measurement is substantially lower than previous estimates for such systems, providing constraints on physical models of accretion physics in black hole and neutron star binary systems.