High-resolution rotation curves of low surface brightness galaxies

By W. D. de Blok, A. Bosma. 2002

701 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/8e1b14e6f490034dca136b1cc651baa054af0240

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Citations in the corpus

SPARC: MASS MODELS FOR 175 DISK GALAXIES WITH SPITZER PHOTOMETRY AND ACCURATE ROTATION CURVES (2016, methodology): “The raw Hα data are typically fit with a spline to derive smooth rotation curves (de Blok et al. 2001; de Blok & Bosma 2002; Noordermeer et al. 2007), which average over small-scale irregularities and trace the overall gravitational potential.”
Empirical Models for Dark Matter Halos. II. Inner Profile Slopes, Dynamical Profiles, and ρ/σ3 (2006, methodology): “Figure 11 shows the logarithmic slope of this model, together with data from de Blok et al. (2001), de Blok & Bosma (2002), and Swaters et al. (2003a) for which values of the scale radius rc were available.”
NIHAO – IV: core creation and destruction in dark matter density profiles across cosmic time (2015, background): “…data are split in three groups, the grey symbols areresults from dwarf and Low Surface Brightness (LSB) galaxies (de Blok et al. 2001; de Blok & Bosma 2002; Swaters et al. 2003), cyan filled squares are the results from the THINGS survey (Oh et al. 2011a), while open blue squares with…”
A KINEMATIC STUDY OF THE ANDROMEDA DWARF SPHEROIDAL SYSTEM (2013, background): “…predicted by cosmological simulations (Navarro et al. 1997), or constant density cores, similar to what is observed in low surface brightness galaxies (Blais-Ouellette et al. 2001; de Blok & Bosma 2002; de Blok et al. 2003; de Blok 2005; Swaters et al. 2003; Kassin et al. 2006; Spano et al. 2008).”
Structure of Disk-dominated Galaxies. II. Color Gradients and Stellar Population Models (2004, methodology): “…i line widths were collected from various sources in the literature: Courteau (1996) (seven galaxies); Bottinelli et al. (1990) (74 galaxies); Theureau et al. (1998) (11 galaxies); Haynes et al. (1999) (one galaxy); de Blok & Bosma (2002) (one galaxy); de Blok et al. (2001) (four galaxies).”
The unexpected diversity of dwarf galaxy rotation curves (2015, positive): “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”
Rotation Curves of Spiral Galaxies (2000, background): “Recent optical rotation curves (Swaters 1999, 2001; Swaters et al. 2000; de Blok et al. 2001) reveal a steeper rise for some, but not all, of the galaxies studied previously at 21-cm.”
A Bird's Eye View of f (R)-Gravity (2009, methodology): “Our sample contains fifteen LSB galaxies with data on the rotation curve, the surface mass density of the gas component and R -band disk photometry extracted from a larger sample selected by de Blok & Bosma [121].”
The Dwarf Galaxy DDO 47 as a Dark Matter Laboratory: Testing Cusps Hiding in Triaxial Halos (2005, background): “…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, McGaugh & Rubin 2001, Salucci 2001, de Blok & Bosma 2002, Weldrake et al. 2003, Gentile et al. 2004).”
One Law to Rule Them All: The Radial Acceleration Relation of Galaxies (2016, background): “The ΛCDM model is known to face severe problems with both the rotation curves of disk galaxies (e.g., Moore et al. 1999; de Blok et al. 2001; McGaugh et al. 2007; Kuzio de Naray et al. 2009) and the dynamics of dSphs (e.g., Boylan-Kolchin et al. 2011; Walker & Peñarrubia 2011; Pawlowski et al.…”
The Dark Matter Distribution in the Central Regions of Galaxy Clusters: Implications for Cold Dark Matter (2003, result): “Some studies have provided evidence for cores of roughly constant density (e.g. de Blok et al. 2001; de Blok & Bosma 2002; Simon et al. 2003) whereas others find their data are consistent with β=1 (e.g. van den Bosch & Swaters 2001; Swaters et al. 2003).”
Stellar Populations in the Nuclei of Late-Type Spiral Galaxies (2006, background): “It is not clear why that should be so, as rotation curve measurements of galaxies of similar type show that their gravitational potentials are shallow, i.e. the gravitational vector vanishes at the center (e.g. de Blok et al. 2001a, 2001b, Matthews & Gallagher 2002, Marchesini et al. 2002).”