Matches in SemOpenAlex for { <https://semopenalex.org/work/W3137245188> ?p ?o ?g. }
- W3137245188 endingPage "160" @default.
- W3137245188 startingPage "160" @default.
- W3137245188 abstract "We present Tully-Fisher distances for 24 AGN host galaxies with black hole mass ($M_textrm{{BH}}$) measurements from reverberation mapping, as well as the first calibration of the $V-$band Tully-Fisher relation. Combining our measurements of HI 21cm emission with $HST$ and ground-based optical and near-infrared images allows multiple distance measurements for 19 galaxies and single measurements for the remaining 5. Separation of the nucleus from its host galaxy via surface brightness decomposition yields galaxy-only luminosities, thus allowing measurements of the distance moduli free of contamination from the AGN. For 14 AGN hosts, these are the first reported distances independent of redshift, and hence independent of peculiar velocities. For the remaining galaxies, we show good agreement between our distances and those previously reported from surface brightness fluctuations (SBF) and Cepheids. We also determine the total galaxy mass enclosed within the estimated HI radius, which when compared to the baryonic content allows for constraints on the dark matter masses. We find a typical mass fraction of $M_{textrm{DM}}$/$M_{textrm{DYN}}$ = 62%, and find significant correlations between $M_{textrm{BH}}$ $-$ $M_{textrm{DYN}}$ and $M_{textrm{BH}}$ $-$ $M_{textrm{DM}}$. Finally, we scale our galaxy radii based on estimated relationships between visible and halo radii and assume a flat rotation curve out to the halo radius to approximate $M_{textrm{HALO}}$. Over the range of $M_{textrm{BH}}$ and $M_{textrm{HALO}}$ in this sample, we find good agreement with observationally-constrained relationships between $M_{textrm{BH}}$ and $M_{textrm{HALO}}$ and with hydrodynamical simulations." @default.
- W3137245188 created "2021-03-29" @default.
- W3137245188 creator A5014347419 @default.
- W3137245188 creator A5019323018 @default.
- W3137245188 creator A5038913587 @default.
- W3137245188 creator A5043601084 @default.
- W3137245188 creator A5056728994 @default.
- W3137245188 creator A5063259408 @default.
- W3137245188 creator A5070481347 @default.
- W3137245188 creator A5070767527 @default.
- W3137245188 creator A5091590493 @default.
- W3137245188 date "2021-05-01" @default.
- W3137245188 modified "2023-09-30" @default.
- W3137245188 title "Tully–Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-mapped AGNs" @default.
- W3137245188 cites W1839080075 @default.
- W3137245188 cites W1892812743 @default.
- W3137245188 cites W1955148565 @default.
- W3137245188 cites W1968187369 @default.
- W3137245188 cites W1971420501 @default.
- W3137245188 cites W1980547824 @default.
- W3137245188 cites W1980708053 @default.
- W3137245188 cites W1983324554 @default.
- W3137245188 cites W1986751831 @default.
- W3137245188 cites W1999532189 @default.
- W3137245188 cites W2000878451 @default.
- W3137245188 cites W2006878995 @default.
- W3137245188 cites W2007344832 @default.
- W3137245188 cites W2013618456 @default.
- W3137245188 cites W2016759553 @default.
- W3137245188 cites W2017775162 @default.
- W3137245188 cites W2023344562 @default.
- W3137245188 cites W2024846775 @default.
- W3137245188 cites W202638490 @default.
- W3137245188 cites W2026489525 @default.
- W3137245188 cites W2026637613 @default.
- W3137245188 cites W2027581992 @default.
- W3137245188 cites W2029343094 @default.
- W3137245188 cites W2031582484 @default.
- W3137245188 cites W2033599776 @default.
- W3137245188 cites W2033803356 @default.
- W3137245188 cites W2037744399 @default.
- W3137245188 cites W2038207393 @default.
- W3137245188 cites W2042905846 @default.
- W3137245188 cites W2045759471 @default.
- W3137245188 cites W2047574411 @default.
- W3137245188 cites W2047862113 @default.
- W3137245188 cites W2048586286 @default.
- W3137245188 cites W2051090249 @default.
- W3137245188 cites W2052247350 @default.
- W3137245188 cites W2057954537 @default.
- W3137245188 cites W2058613207 @default.
- W3137245188 cites W2060839332 @default.
- W3137245188 cites W2062237753 @default.
- W3137245188 cites W2062540759 @default.
- W3137245188 cites W2063000920 @default.
- W3137245188 cites W2068962850 @default.
- W3137245188 cites W2070444660 @default.
- W3137245188 cites W2070630406 @default.
- W3137245188 cites W2074085035 @default.
- W3137245188 cites W2074187822 @default.
- W3137245188 cites W2074760579 @default.
- W3137245188 cites W2079227246 @default.
- W3137245188 cites W2082161920 @default.
- W3137245188 cites W2086746632 @default.
- W3137245188 cites W2087517229 @default.
- W3137245188 cites W2089750221 @default.
- W3137245188 cites W2090459210 @default.
- W3137245188 cites W2093318533 @default.
- W3137245188 cites W2095424371 @default.
- W3137245188 cites W2096623050 @default.
- W3137245188 cites W2103474895 @default.
- W3137245188 cites W2106873657 @default.
- W3137245188 cites W2109353143 @default.
- W3137245188 cites W2111817932 @default.
- W3137245188 cites W2115468377 @default.
- W3137245188 cites W2128089313 @default.
- W3137245188 cites W2133376928 @default.
- W3137245188 cites W2135894620 @default.
- W3137245188 cites W2136336431 @default.
- W3137245188 cites W2136741290 @default.
- W3137245188 cites W2147981121 @default.
- W3137245188 cites W2153408444 @default.
- W3137245188 cites W2159478752 @default.
- W3137245188 cites W2208735541 @default.
- W3137245188 cites W2263568668 @default.
- W3137245188 cites W2346927002 @default.
- W3137245188 cites W2527843097 @default.
- W3137245188 cites W2561067311 @default.
- W3137245188 cites W2625830509 @default.
- W3137245188 cites W2767435318 @default.
- W3137245188 cites W2787779748 @default.
- W3137245188 cites W2885255958 @default.
- W3137245188 cites W2907825931 @default.
- W3137245188 cites W2910458756 @default.
- W3137245188 cites W2913673361 @default.
- W3137245188 cites W2938388504 @default.
- W3137245188 cites W2949744235 @default.
- W3137245188 cites W2963193352 @default.