Zobrazeno 1 - 10
of 2 208
pro vyhledávání: '"Smith, Mark D."'
Autor:
Zhang, Hengyue, Bureau, Martin, Smith, Mark D., Cappellari, Michele, Davis, Timothy A., Dominiak, Pandora, Elford, Jacob S., Liang, Fu-Heng, Ruffa, Ilaria, Williams, Thomas G.
The mass ($M_\mathrm{BH}$) of a supermassive black hole (SMBH) can be measured using spatially-resolved kinematics of the region where the SMBH dominates gravitationally. The most reliable measurements are those that resolve the smallest physical sca
Externí odkaz:
http://arxiv.org/abs/2404.16345
Autor:
Cromhout, Markus
Publikováno v:
Neotestamentica, 2019 Jan 01. 53(3), 602-608.
Externí odkaz:
https://www.jstor.org/stable/26887860
Autor:
Liang, Fu-Heng, Smith, Mark D., Bureau, Martin, Gao, Feng, Davis, Timothy A., Cappellari, Michele, Elford, Jacob S., Greene, Jenny E., Iguchi, Satoru, Lelli, Federico, Lu, Anan, Ruffa, Ilaria, Williams, Thomas G., Zhang, Hengyue
The co-evolution of galaxies and supermassive black holes (SMBHs) underpins our understanding of galaxy evolution, but different methods to measure SMBH masses have only infrequently been cross-checked. We attempt to identify targets to cross-check t
Externí odkaz:
http://arxiv.org/abs/2311.15447
Autor:
Lelli, Federico, Davis, Timothy A., Bureau, Martin, Cappellari, Michele, Liu, Lijie, Ruffa, Ilaria, Smith, Mark D., Williams, Thomas G.
The mm-Wave Interferometric Survey of Dark Object Masses (WISDOM) is probing supermassive black holes (SMBHs) in galaxies across the Hubble sequence via molecular gas dynamics. We present the first WISDOM study of a luminous infrared galaxy with an a
Externí odkaz:
http://arxiv.org/abs/2209.00363
Autor:
Tang, Yinghua, Ebadi, Mehrnoosh, Lei, Junying, Feng, Zehua, Fakhari, Shahab, Wu, Peipei, Smith, Mark D., Limberis, Maria P., Kolbeck, Roland, Excoffon, Katherine J., Yan, Ziying, Engelhardt, John F.
Publikováno v:
In Molecular Therapy - Methods & Clinical Development 13 June 2024 32(2)
Autor:
North, Eve V., Davis, Timothy A., Bureau, Martin, Gaspari, Massimo, Cappellari, Michele, Iguchi, Satoru, Liu, Lijie, Onishi, Kyoko, Sarzi, Marc, Smith, Mark D., Williams, Thomas G.
We present high-resolution (synthesised beam size 0."088x0."083 or 25x23 pc$^2$) Atacama Large Millimetre/submillimetre Array (ALMA) $^{12}$CO(2-1) line and 236 GHz continuum observations, as well as 5 GHz enhanced Multi-Element Radio Linked Interfer
Externí odkaz:
http://arxiv.org/abs/2103.08988
Autor:
Smith, Mark D., Bureau, Martin, Davis, Timothy A., Cappellari, Michele, Liu, Lijie, Onishi, Kyoko, Iguchi, Satoru, North, Eve V., Sarzi, Marc, Williams, Thomas G.
Supermassive black hole (SMBH) masses can be measured by resolving the dynamical influences of the SMBHs on spatially-resolved tracers of the central potentials. Modern long-baseline interferometers have enabled the use of molecular gas as such a tra
Externí odkaz:
http://arxiv.org/abs/2103.08920
Autor:
Smith, Mark D., Bureau, Martin, Davis, Timothy A., Cappellari, Michele, Liu, Lijie, Onishi, Kyoko, Iguchi, Satoru, North, Eve V., Sarzi, Marc
Empirical correlations between the masses of supermassive black holes (SMBHs) and properties of their host galaxies are well-established. Among these is the correlation with the flat rotation velocity of each galaxy measured either at a large radius
Externí odkaz:
http://arxiv.org/abs/2010.08565
Autor:
Davis, Timothy A., Nguyen, Dieu D., Seth, Anil C., Greene, Jenny E., Nyland, Kristina, Barth, Aaron J., Bureau, Martin, Cappellari, Michele, Brok, Mark den, Iguchi, Satoru, Lelli, Federico, Liu, Lijie, Neumayer, Nadine, North, Eve V., Onishi, Kyoko, Sarzi, Marc, Smith, Mark D., Williams, Thomas G.
We estimate the mass of the intermediate-mass black hole at the heart of the dwarf elliptical galaxy NGC 404 using Atacama Large Millimeter/submillimeter Array (ALMA) observations of the molecular interstellar medium at an unprecedented linear resolu
Externí odkaz:
http://arxiv.org/abs/2007.05536