Kinematical data on early-type galaxies. VI

By F. Simien, P. Prugniel. 2002

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In Astronomy and Astrophysics

Citations in the corpus

DISSIPATION AND EXTRA LIGHT IN GALACTIC NUCLEI. II. “CUSP” ELLIPTICALS (2008, methodology): “The details of the fitting for our simulations are described in Cox et al. (2006b), and for the observations in Bender et al. (1987, 1992), Bender (1988), Faber et al. (1989), Simien & Prugniel (1997), and Simien & Prugniel (2002).”
Star Formation Histories of Early-Type Galaxies. I. Higher Order Balmer Lines as Age Indicators (2003, result): “For the low- galaxies ( < 80 km s 1), our values tend to be systematically higher by about 50% than the recent values determined by Simien & Prugniel (2002), Pedraz et al. (2002), and Geha, Guhathakurta, & van der Marel (2002).”
Spectroscopic ages and metallicities of stellar populations : validation of full spectrum fitting (2008, methodology): “At variance, our approach does not affect the real spectral features, it is rather similar to the method of Simien & Prugniel (like in Simien & Prugniel 2002) that renormalises the observations using a polynomial fitted on the ratio between the observation and the best model and iterate until…”
THE 2MASS REDSHIFT SURVEY—DESCRIPTION AND DATA RELEASE (2011, unknown): “…1997A&AS..123..411M Maurogordato et al. (1997) 1997A&AS..125..247Q Quintana et al. (1997) 1997A&AS..125..329d de Souza et al. (1997) 1997A&AS..126...15S Simien & Prugniel (1997b) 1997A&AS..126..519S Simien & Prugniel (1997c) 1997ApJ...478..107P Pence & Rots (1997) 1997ApJ...478..144S Solomon…”
Internal Dynamics, Structure, and Formation of Dwarf Elliptical Galaxies. II. Rotating versus Nonrotating Dwarfs (2002, background): “In several of our figures, we include two additional galaxies, VCC 1122 and VCC 1407 (Simien & Prugniel 2002).”
Properties of Globular Cluster Systems in Nearby Early-Type Galaxies (2001, background): “NGC 4552 This Virgo elliptical is also known as M89, and is known to posses a kinematically distinct core (Simien & Prugniel 1997).”
Kinematic properties of early-type galaxy haloes using planetary nebulae (2008, background): “Stellar kinematics are taken from Debattista, Corsini & Aguerri (2002) for the major axis and Simien & Prugniel (1997) for the minor axis.”
A Fundamental plane of black hole activity (2003, methodology): “We assign black hole masses to these systems using the observed correlation between black hole masses and stellarv ocity dispersion (Gebhardt et al. 2000; Ferrarese & Merritt 2000) 2, mostly using the values of the velocity dispersion providedby the HYPERLEDA catalogue (Simien & Prugniel 2002).”
Virgo Cluster Early-Type Dwarf Galaxies with the Sloan Digital Sky Survey. II. Early-Type Dwarfs with Central Star Formation (2006, unknown): “…et al. (1992); Binggeli et al. (1993); Young & Currie (1995); Drinkwater et al. (1996); Grogin et al. (1998); Falco et al. (1999); Gavazzi et al. (2000); van Driel et al. (2000); Conselice et al. (2001); Simien & Prugniel (2002); Caldwell et al. (2003); Geha et al. (2003); Gavazzi et al. (2004).”
STRUCTURE AND FORMATION OF ELLIPTICAL AND SPHEROIDAL GALAXIES (2008, methodology): “Simien & Prugniel (1997, 1998) took spectra of NGC 4318 using the 1.93 m telescope of the Observatoire de Haute-Provence.”
Accurate masses for dispersion-supported galaxies (2009, background): “…(1998), x) McConnachie et al. (2005), y) Simien & Prugniel (2002), z) Quoted from NASA/IPAC Extragalactic Database, aa) Simien & Prugniel (2000), bb) Simien & Prugniel (1997c), cc) Simien & Prugniel (1997b), dd) Kormendy et al. (2009), who present similar parameters to those the originally…”
A REVISED PARALLEL-SEQUENCE MORPHOLOGICAL CLASSIFICATION OF GALAXIES: STRUCTURE AND FORMATION OF S0 AND SPHEROIDAL GALAXIES (2011, background): “More generally, some Sphs rotate rapidly (de Rijcke et al. 2001; Simien & Prugniel 2002; Pedraz et al. 2002; Tolstoy et al. 2009); others do not (Geha et al. 2003; Thomas et al. 2006).”