Surface BR Photometry of Newly Discovered Dwarf Elliptical Galaxies in the Nearby Sculptor and Centaurus A Groups

By H. Jerjen, B. Binggeli, Kenneth C. Freeman. 2000

136 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/5cb29632f3d927610ec2ede15c54836fa0df0c1c

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In Astronomy and Astrophysics

In Instrumentation

Citations in the corpus

A Catalog of Neighboring Galaxies (2004, unknown): “33 34 03 Karachentsev et al. 2002b; ph: Jerjen et al. 2000a 13 24 36.0......”
Inclination- and dust-corrected galaxy parameters: bulge-to-disc ratios and size–luminosity relations (2008, background): “Dwarf elliptical galaxies also have values of n < 2 (e.g. Caon et al. 1993; Young & Currie 1994; Jerjen et al. 2000) — they define the low-mass end of a linear relation between magnitude and Sérsic index (e.g. Graham et al. 2006b, their figure 1; Nipoti, Londrillo & Ciotti 2006).”
Evidence for a New Elliptical-Galaxy Paradigm: Sérsic and Core Galaxies (2004, background): “Since the Sérsic shape parameter n is correlated with luminosity (e.g., Caon et al. 1993; Jerjen et al. 2000; Graham & Guzmán 2003) and with central velocity dispersion (Graham et al. 2001a; Graham 2002), we have a natural explanation for the correlation between and luminosity: Sérsic profiles…”
New distances to galaxies in the Centaurus A group (2002, methodology): “Distances had been estimated only for the brightest galaxies in the group until Jerjen et al. (2000a) applied the method of surface brightness fluctuations to measure distances to five dwarf galaxies in the Centaurus A group.”
Palomar/Las Campanas Imaging Atlas of Blue Compact Dwarf Galaxies. I. Images and Integrated Photometry (2003, background): “This figure shows the PSB of BCDs being significantly brighter than that of dIrr (Parodi et al. 2002; Patterson & Thuan 1996) and dE (Jerjen et al. 2000).”
A New Empirical Model for the Structural Analysis of Early-Type Galaxies, and A Critical Review of the Nuker Model (2003, background): “…of describing both the outer and the inner profiles (with a point source used by Graham &Guzmán to fit those galaxies that are nucleated), and since Jerjen et al. (2000) were able to fit the highly resolved (because of their proximity) Milky Way andM31 dwarf spheroidal profiles at all radii…”
The Hubble Flow around the Centaurus A/M83 Galaxy Complex (2006, methodology): “Its optical spectrum shows emission lines with a mean velocity of +741 km s 1 (Jerjen et al. 2000a).”