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• W1915403750 endingPage "1816" @default.
• W1915403750 startingPage "1792" @default.
• W1915403750 abstract "We present a dynamical analysis to infer the structural parameters and properties of the two nearby, compact, high velocity dispersion galaxies MRK1216 & NGC1277. Combining deep HST imaging, wide-field IFU stellar kinematics, and complementary long-slit spectroscopic data out to 3 R_e, we construct orbit-based models to constrain their black hole masses, dark matter content and stellar mass-to-light ratios. We obtain a black hole mass of log(Mbh/Msun) = 10.1(+0.1/-0.2) for NGC1277 and an upper limit of log(Mbh/Msun) = 10.0 for MRK1216, within 99.7 per cent confidence. The stellar mass-to-light ratios span a range of Upsilon_V = 6.5(+1.5/-1.5) in NGC1277 and Upsilon_H = 1.8(+0.5/-0.8) in MRK1216 and are in good agreement with SSP models of a single power-law Salpeter IMF. Even though our models do not place strong constraints on the dark halo parameters, they suggest that dark matter is a necessary ingredient in MRK1216, with a dark matter contribution of 22(+30/-20) per cent to the total mass budget within 1 R_e. NGC1277, on the other hand, can be reproduced without the need for a dark halo, and a maximal dark matter fraction of 13 per cent within the same radial extent. In addition, we investigate the orbital structures of both galaxies, which are rotationally supported and consistent with photometric multi-S'ersic decompositions, indicating that these compact objects do not host classical, non-rotating bulges formed during recent (z <= 2) dissipative events or through violent relaxation. Finally, both MRK 1216 and NGC 1277 are anisotropic, with a global anisotropy parameter delta of 0.33 and 0.58, respectively. While MRK 1216 follows the trend of fast-rotating, oblate galaxies with a flattened velocity dispersion tensor in the meridional plane of the order of beta_z = delta, NGC 1277 is highly tangentially anisotropic and seems to belong kinematically to a distinct class of objects." @default.
• W1915403750 created "2016-06-24" @default.
• W1915403750 creator A5001553407 @default.
• W1915403750 creator A5023699178 @default.
• W1915403750 creator A5026266948 @default.
• W1915403750 creator A5033875500 @default.
• W1915403750 creator A5038068614 @default.
• W1915403750 creator A5051770664 @default.
• W1915403750 creator A5054559636 @default.
• W1915403750 creator A5078390799 @default.
• W1915403750 date "2015-07-17" @default.
• W1915403750 modified "2023-09-30" @default.
• W1915403750 title "MRK 1216 and NGC 1277 – an orbit-based dynamical analysis of compact, high-velocity dispersion galaxies" @default.
• W1915403750 cites W1490779553 @default.
• W1915403750 cites W1491361171 @default.
• W1915403750 cites W1499069497 @default.
• W1915403750 cites W1520641405 @default.
• W1915403750 cites W1560414242 @default.
• W1915403750 cites W1862292818 @default.
• W1915403750 cites W1865864028 @default.
• W1915403750 cites W1956191709 @default.
• W1915403750 cites W1971074558 @default.
• W1915403750 cites W1978594376 @default.
• W1915403750 cites W1979503956 @default.
• W1915403750 cites W1980547824 @default.
• W1915403750 cites W1983938604 @default.
• W1915403750 cites W1984716389 @default.
• W1915403750 cites W1988245473 @default.
• W1915403750 cites W1989222696 @default.
• W1915403750 cites W1989983328 @default.
• W1915403750 cites W1990401433 @default.
• W1915403750 cites W1993015838 @default.
• W1915403750 cites W1993080318 @default.
• W1915403750 cites W1994671833 @default.
• W1915403750 cites W2000423827 @default.
• W1915403750 cites W2003814700 @default.
• W1915403750 cites W2003926479 @default.
• W1915403750 cites W2008999029 @default.
• W1915403750 cites W2009415789 @default.
• W1915403750 cites W2013985911 @default.
• W1915403750 cites W2015305364 @default.
• W1915403750 cites W2016094316 @default.
• W1915403750 cites W2017723918 @default.
• W1915403750 cites W2019850329 @default.
• W1915403750 cites W2023344562 @default.
• W1915403750 cites W2025020969 @default.
• W1915403750 cites W2026132224 @default.
• W1915403750 cites W2029343094 @default.
• W1915403750 cites W2030594902 @default.
• W1915403750 cites W2031617522 @default.
• W1915403750 cites W2033185246 @default.
• W1915403750 cites W2034288205 @default.
• W1915403750 cites W2037816996 @default.
• W1915403750 cites W2038820954 @default.
• W1915403750 cites W2038900887 @default.
• W1915403750 cites W2040759695 @default.
• W1915403750 cites W2041030011 @default.
• W1915403750 cites W2041211839 @default.
• W1915403750 cites W2041764991 @default.
• W1915403750 cites W2042516441 @default.
• W1915403750 cites W2046999656 @default.
• W1915403750 cites W2048025997 @default.
• W1915403750 cites W2054878344 @default.
• W1915403750 cites W2056859889 @default.
• W1915403750 cites W2062345471 @default.
• W1915403750 cites W2062509935 @default.
• W1915403750 cites W2064776492 @default.
• W1915403750 cites W2066645046 @default.
• W1915403750 cites W2070887798 @default.
• W1915403750 cites W2073032833 @default.
• W1915403750 cites W2073152836 @default.
• W1915403750 cites W2077054687 @default.
• W1915403750 cites W2079227246 @default.
• W1915403750 cites W2082108152 @default.
• W1915403750 cites W2084691636 @default.
• W1915403750 cites W2084780057 @default.
• W1915403750 cites W2085390946 @default.
• W1915403750 cites W2086348625 @default.
• W1915403750 cites W2086535097 @default.
• W1915403750 cites W2088034685 @default.
• W1915403750 cites W2088392768 @default.
• W1915403750 cites W2089873313 @default.
• W1915403750 cites W2090192186 @default.
• W1915403750 cites W2090482424 @default.
• W1915403750 cites W2091765531 @default.
• W1915403750 cites W2092569776 @default.
• W1915403750 cites W2097690225 @default.
• W1915403750 cites W2098914923 @default.
• W1915403750 cites W2100479967 @default.
• W1915403750 cites W2100665021 @default.
• W1915403750 cites W2101317783 @default.
• W1915403750 cites W2105954496 @default.
• W1915403750 cites W2112633422 @default.
• W1915403750 cites W2117335531 @default.
• W1915403750 cites W2122952850 @default.
• W1915403750 cites W2126515197 @default.
• W1915403750 cites W2126805297 @default.
• W1915403750 cites W2130044662 @default.

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