High-Resolution Rotation Curves of Low Surface Brightness Galaxies. II. Mass Models

By W. D. de Blok, S. McGaugh, Vera C. Rubin. 2001

157 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Global and Planetary Change

View Paper: https://www.semanticscholar.org/paper/e82014f8bbae51438830405e2ea81e0e5c399d66

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. S. McGaugh
2. P. Hopkins
3. J. Schombert
4. L. Hernquist
5. A. Dutton
6. A. Dekel
7. Volker Springel
8. F. Walter

In Global and Planetary Change

1. W. J. Blok
2. F. Lelli
3. J. Schombert
4. A. Dutton
5. A. Macciò
6. A. Bosma
7. W. D. de Blok
8. S. McGaugh

Citations in the corpus

• The rotation curves shapes of late-type dwarf galaxies (2009, background): “…Blok et al. 1996; de Blok & McGaugh 1997; Stil 1999; Swaters 1999; Swaters et al. 2000; van den Bosch et al. 2001; van den Bosch & Swaters 2001; de Blok et al. 2001; Marchesini et al. 2002; de Blok & Bosma 2002, herafter dBB; Swaters et al. 2003a, hereafter SMvdBB; Rhee et al. 2004; Simon et al.…”
• Convergence and scatter of cluster density profiles (2004, background): “This is especially timely given the abundance of new highresolution data that probe the central structure of galaxies (e.g. de Blok et al. 2001a; de Blok, McGaugh & Rubin 2001b; McGaugh, Rubin & de Blok 2001; de Blok & Bosma 2002; Swaters et al. 2003) and clusters (e.g. Sand et al. 2004).”
• The Dwarf Galaxy DDO 47 as a Dark Matter Laboratory: Testing Cusps Hiding in Triaxial Halos (2005, background): “…that in a large number of cases, the inferred cores of dark matter halos are much shallower than expected from the NFW fit (Flores & Primack 1994; Moore 1994; Burkert 1995; Salucci & Burkert 2000; de Blok et al. 2001; Salucci 2001; de Blok & Bosma 2002; Weldrake et al. 2003; Gentile et al. 2004).”
• The DiskMass Survey VII. The distribution of luminous and dark matter in spiral galaxies (2013, background): “Observationally, however, a core-like density distribution is often inferred (de Blok et al. 2001; Swaters et al. 2003a,b; Kuzio de Naray et al. 2008, 2009; de Blok 2010; Oh et al. 2011).”
• The unexpected diversity of dwarf galaxy rotation curves (2015, unknown): “The advent of two-dimensional observational surveys with better sensitivity and angular resolution have allayed some of these earlier concerns (e.g. Simon et al. 2003; de Blok et al. 2008; Kuzio de Naray, McGaugh & de Blok 2008; Oh et al. 2011, 2015; Adams et al. 2014), and have led to the view that”
• High-resolution rotation curves of low surface brightness galaxies (2002, methodology): “Rather, the rotation curves prefer a pseudo-isothermal (i.e. core-dominated) halo model. de Blok et al. (2001b) furthermore showed that all rotation curves of LSB galaxies measured so far are consistent with a pseudo-isothermal core model.”
• SPARC: MASS MODELS FOR 175 DISK GALAXIES WITH SPITZER PHOTOMETRY AND ACCURATE ROTATION CURVES (2016, methodology): “…of objects excluding duplicates): Swaters et al. (2009, 32), Sanders & Verheijen (1998, 30), Sanders (1996, 17), Noordermeer et al. (2007, 12), de Blok et al. (2001, 10), Begeman et al. (1991, 9), Lelli et al. (2012a,b, 2014, 8), de Blok & Bosma (2002, 7), de Blok et al. (1996, 7), Kuzio de…”
• Concentration, spin and shape of dark matter haloes as a function of the cosmological model: WMAP1, WMAP3 and WMAP5 results (2008, background): “…between the inner density slopes of dwarf and LSB galaxies and those predicted by CDM (e.g., Moore 1994; Flores & Primack 1994; van den Bosch & Swaters 2001; de Blok et al. 2001, 2002; Swaters et al. 2003, Dutton et al. 2005; Gentile et al. 2005; Simon et al. 2005; Kuzio de Naray et al. 2008).”
• A high-resolution rotation curve of NGC 6822 (2002, methodology): “In de Blok et al. (2001b) the inner mass density slopes of a large sample of LSB galaxies was derived, and the most representative value was α = −0.2± 0.2, i.e. closer to pseudo-isothermal than to CDM.”