Orbital structure and mass distribution in elliptical galaxies

By A. Kronawitter, R. Saglia, O. Gerhard, R. Bender. 2000

197 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/9274197dc4702886f9ffe7ba84a918936c4c2c53

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In Astronomy and Astrophysics

1. M. Cappellari
2. P. Hopkins
3. L. Hernquist
4. Thomas J. Cox
5. T. Naab
6. Luis C. Ho
7. Volker Springel
8. C. Conroy

In Instrumentation

1. M. Cappellari
2. P. Hopkins
3. L. Hernquist
4. Thomas J. Cox
5. Luis C. Ho
6. T. Naab
7. Volker Springel
8. J. Kormendy

Citations in the corpus

• Properties of spherical galaxies and clusters with an NFW density profile (2000, background): “On the other hand, Kronawitter et al. (2000) are able to rule out constant Υ for some elliptical galaxies.”
• The Phase-Space Density Profiles of Cold Dark Matter Halos (2001, background): “…lensing of galaxies and clusters (see, e.g., Tyson, Kochanski & dell’Antonio 1998, Williams, Navarro & Bartelmann 1999), and by detailed studies of the stellar dynamics of spheroidal galaxies (Carollo et al. 1995; Rix et al. 1997; Gerhard et al. 1998; Cretton et al. 2000; Kronawitter et al. 2000).”
• THE SINFONI BLACK HOLE SURVEY: THE BLACK HOLE FUNDAMENTAL PLANE REVISITED AND THE PATHS OF (CO)EVOLUTION OF SUPERMASSIVE BLACK HOLES AND BULGES (2016, methodology): “…/L , D=18.8 Mpc from Atkinson et al. (2005), not corrected for G.E., AV = 0.1, AR = 0.081, (V − F606W ) = 0.36 NGC1399 M/LB = 10.2M /L , D=21.1 Mpc from Kronawitter et al. (2000), G.E. corrected NGC2273 M/LR derived fitting the stellar kinematics of Greene et al. (2010), AR = 0.189 NGC2549 M/LR…”
• The SLUGGS Survey: kinematics for over 2500 globular clusters in 12 early-type galaxies (2012, methodology): “The dynamics of NGC 5846 has been modelled within 1Reff (Kronawitter et al. 2000; Cappellari et al. 2007).”
• A Theoretical Interpretation of the Black Hole Fundamental Plane (2007, methodology): “Observationally, a similar mean correlation (σ ≈ 0.66vmax, nearly identical to the bestfit normalization in our simulations; e.g. Kronawitter et al. 2000; Gerhard et al. 2001) is found.”
• The Dark Matter Distribution in the Central Regions of Galaxy Clusters: Implications for Cold Dark Matter (2003, background): “From an observational point of view, Kronawitter et al. (2000) found that in their sample of galaxies the best-fitting models were nearly isotropic with typical α ≃ 0.3 (α is the anisotropy parameter, see Appendix Eqn.”
• Kinematic properties of early-type galaxy haloes using planetary nebulae (2008, unknown): “Mass modelling of NGC 5846 has been performed by van der Marel (1991), Kronawitter et al. (2000), Cappellari et al. (2007), all using stellar kinematics within 1 effective radius.”
• STRUCTURE AND FORMATION OF ELLIPTICAL AND SPHEROIDAL GALAXIES (2008, methodology): “They include additionalM/L values based on three-integral models (Gebhardt et al. 2003, 2007; Thomas et al. 2007), two-integral models of galaxies observed to very large radii (Kronawitter et al. 2000; Gerhard et al. 2001), and two-integral models of large galaxy samples (e. g., van der Marel 1991).”
• The Sloan Lens ACS Survey. IV. The Mass Density Profile of Early-Type Galaxies out to 100 Effective Radii (2007, result): “In addition, the “mean” fraction of DM fdm,3D(< Reff) ∼ 30% is in excellent agreement with local estimates (Kronawitter et al. 2000; Gerhard et al. 2001; Borriello et al. 2003), and more recently from the SAURON project (Cappellari et al. 2006).”
• DISSECTING THE GRAVITATIONAL LENS B1608+656. II. PRECISION MEASUREMENTS OF THE HUBBLE CONSTANT, SPATIAL CURVATURE, AND THE DARK ENERGY EQUATION OF STATE (2009, background): “The inner cutoff of rani is motivated by observations (e.g., Kronawitter et al. 2000) and radial instability arguments (e.g., Merritt & Aguilar 1985; Stiavelli & Sparke 1991), while the outer cutoff is for computational simplicity (the model velocity dispersion changes by a negligible amount…”
• The Fundamental Scaling Relations of Elliptical Galaxies (2005, background): “…Prugniel & Simien 1994; Pahre et al. 1995, 1998a, 1998b; Prugniel & Simien 1996; Busarello et al. 1997; Graham & Colless 1997; Mobasher et al. 1999; Kronawitter et al. 2000; Gerhard et al. 2001; Bernardi et al. 2003a; Padmanabhan et al. 2004; Woo et al. 2004; Cappellari et al. 2006) and extended…”
• The Structure and Dynamics of Luminous and Dark Matter in the Early-Type Lens Galaxy of 0047–281 at z = 0.485 (2002, background): “…description for computing kinematic quantities of E/S0 galaxies with axis ratio b=a 0:8, like 0047 281 (see, e.g., Saglia, Bertin, & Stiavelli 1992; Kronawitter et al. 2000), even though clearly they are not appropriate for the lensing analysis, since, e.g., they do not produce quadruply lensed…”
• Axisymmetric Dynamical Models of the Central Regions of Galaxies (2002, background): “It appears that in most elliptical galaxies the dark halo becomes important at about the half-light radius (Kronawitter et al. 2000; Rix et al. 1997).”
• Two-dimensional kinematics of SLACS lenses – III. Mass structure and dynamics of early-type lens galaxies beyond z ≃ 0.1 (2011, background): “…mass-to-light ratios (in theB-band) corresponding to the maximal luminous profiles are in the range 3< M∗/L⊙,B < 10, fully consistent with the values determined for local earlytype galaxies (see e.g. Kronawitter et al. 2000 Gerhard et al. 2001, Trujillo, Burkert, & Bell 2004, Mamon & Łokas 2005).”
• Supermassive Black Holes in Galactic Nuclei: Past, Present and Future Research (2004, methodology): “For the elliptical galaxies, the circular velocity is derived from dynamical models applied to the stellar kinematics (Gerhard et al. 2001; Kronawitter et al. 2000).”
• Density profiles of galaxy groups and clusters from SDSS galaxy–galaxy weak lensing (2006, background): “While the matter distributions in elliptical galaxies can be simply probed on small scales (within a few re) using central velocity dispersions (Kronawitter et al. 2000; de Zeeuw et al. 2002; Padmanabhan et al. 2004), finding probes of the dark matter profiles on larger scales is more challenging.”
• Dynamical modelling of luminous and dark matter in 17 Coma early-type galaxies (2007, background): “So far only one large sample of 21 round, nonrotating giant ellipticals has been probed for dark matter considering at least the full range of spherical models (Kronawitter et al. 2000).”