Dynamics of Galaxies: From the Early Universe to the Present

By F. Combes, G. Mamon, Vassilis Charmandaris. 2000

267 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Computational Mechanics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/63ea5d740960dc10d4fd1e4c827e5f2d4767e267

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. P. Hopkins
2. T. Naab
3. L. Hernquist
4. M. Cappellari
5. Thomas J. Cox
6. Jeremiah P. Ostriker
7. D. Merritt
8. A. Burkert

In Computational Mechanics

1. B. Whitmore
2. D. Merritt
3. S. M. Fall
4. Qing Zhang
5. A. Burkert
6. T. Naab
7. Milos Milosavljevic

In Instrumentation

1. T. Naab
2. M. Cappellari
3. P. Hopkins
4. D. Merritt
5. S. McGaugh
6. A. Burkert
7. L. Hernquist
8. Milos Milosavljevic

Citations in the corpus

• Formation of Galactic Nuclei (2001, methodology): “While the presence of supermassive compact objects has only been reliably established in a handful of galaxies (see discussion in Ferrarese & Merritt 2000), several of the best cases are in stellar systems with steep cusps (e.g., the bulge of the Milky Way; M32).”
• Nested and Single Bars in Seyfert and Non-Seyfert Galaxies (2001, background): “— Galaxy names (col. 1), source of HST data: Mu = Mulchaey; St = Stiavelli; Po = Pogge; Th = Thompson; Ri = Rieke; Sc = Scoville (col. 2), source of outer galaxy data: 2M = 2MASS Sky Survey; DSS = Digital Sky Survey; ING = ING data archive; ESO = ESO data archive; CF = Peletier et al. 1999; Frei = F”
• The Central Mass Distribution in Dwarf and Low Surface Brightness Galaxies (2002, background): “…and on the other hand there are several studies that find that these galaxies are not consistent with steep inner slopes (Borriell & Salucci 2001; Dalcanton & Bernstein 2000; Blais-Ouellette, Amram, & Carignan 2001; de Blok et al. 2001a, hereafter dBMBR; de Blok et al. 2001b, hereafter dBMR; de…”
• Statistical Properties of Collisionless Equal- and Unequal-Mass Merger Remnants of Disk Galaxies (2001, background): “Figure 1 shows the ellipticity profiles for the 3 : 1 merger remnant with”
• Rotation Curves of Spiral Galaxies (2000, background): “Numerous discussions of rotation properties are included in the conference proceedings, Galaxy Dynamics (Merritt et al. 1999), Dynamics of Galaxies (Combes et al. 2000), Galaxy Disks and Disk Galaxies (Funes & Corsini 2001).”
• The Mass Discrepancy-Acceleration Relation: Disk Mass and the Dark Matter Distribution (2004, background): “It is straightforward to derive equivalent limits for other choices of halo models, but most other models resemble one of these two in their essential features.”
• A Multiwavelength Study of the Young Star Clusters and Interstellar Medium in the Antennae Galaxies (2001, methodology): “Repeating the analysis using the Wilson et al. (2000) CO intensity map rather than the BIMA map results in correlations with similar slopes.”
• A Fundamental Relation between Supermassive Black Holes and Their Host Galaxies (2000, unknown): “Values of σ and vr are readily available in the literature (e.g. Prugniel et al. 1998; McElroy 1995).”