J/MNRAS/369/97      M31 planetary nebulae velocities          (Halliday+, 2006)

Planetary nebula velocities in the disc and bulge of M31. Halliday C., Carter D., Bridges T.J., Jackson Z.C., Wilkinson M.I., Quinn D.P., Evans N.W., Douglas N.G., Merrett H.R., Merrifield M.R., Romanowsky A.J., Kuijken K., Irwin M.J. <Mon. Not. R. Astron. Soc., 369, 97-119 (2006)> =2006MNRAS.369...97H 2006MNRAS.369...97H
ADC_Keywords: Galaxies, nearby ; Planetary nebulae ; Radial velocities Keywords: galaxies: haloes - galaxies: individual: M31 - galaxies: spiral Abstract: We present radial velocities for a sample of 721 planetary nebulae in the disc and bulge of M31, measured using the WYFFOS fibre spectrograph on the William Herschel Telescope. Velocities are determined using the [OIII] λ5007 emission line. Rotation and velocity dispersion are measured to a radius of 50arcmin (11.5kpc), the first stellar rotation curve and velocity dispersion profile for M31 to such a radius. Our kinematics are consistent with rotational support at radii well beyond the bulge effective radius of 1.4kpc, although our data beyond a radius of 5kpc are limited. We present tentative evidence for kinematic substructure in the bulge of M31 to be studied fully in a later work. This paper is part of an ongoing project to constrain the total mass, mass distribution and velocity anisotropy of the disc, bulge and halo of M31. Description: Our spectroscopic data were acquired during two observing runs at the William Herschel Telescope, in 1999 August/September and 2001 October. Between our spectroscopic runs we completed an [OIII] plus Stroemgren y imaging survey using the Isaac Newton Telescope (INT) to detect additional PNe targets out to a projected radius of 12kpc. Here and throughout this paper we assume a distance of 770kpc for M31. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 36 40 Positions of a representative selection of fiducial or tertiary astrometric standard stars tablea1.dat 75 721 Positions and velocities of PNe -------------------------------------------------------------------------------- See also: J/ApJ/339/53 : Planetary nebulae as standard candles. II. (Ciardullo+, 1989) J/ApJ/616/804 : Planetary nebulae kinematics in M31 (Hurley-Keller+, 2004) J/MNRAS/369/120 : Kinematic survey of planetary nebulae in M31 (Merrett+, 2006) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Astrometric standard stars designation 12- 13 I2 h RAh Right ascension (J2000) 15- 16 I2 min RAm Right ascension (J2000) 18- 23 F6.3 s RAs Right ascension (J2000) 25 A1 --- DE- Declination sign (J2000) 26- 27 I2 deg DEd Declination (J2000) 29- 30 I2 arcmin DEm Declination (J2000) 32- 36 F5.2 arcsec DEs Declination (J2000) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name PN designation (1) 12- 13 I2 h RAh Right ascension (J2000) 15- 16 I2 min RAm Right ascension (J2000) 18- 22 F5.2 s RAs Right ascension (J2000) 24 A1 --- DE- Declination sign (J2000) 25- 26 I2 deg DEd Declination (J2000) 28- 29 I2 arcmin DEm Declination (J2000) 31- 34 F4.1 arcsec DEs Declination (J2000) 36- 41 F6.1 km/s cz Final heliocentric velocity 43- 46 F4.1 km/s e_cz rms uncertainty on cz 48- 53 F6.2 arcmin Dmaj [-60/72] Distance from the nucleus along major axis (2) 55- 60 F6.2 arcmin Dmin [-48/55] Distance from the nucleus along minor axis (2) 62- 66 F5.2 arcmin Rad Distance from the nucleus 68- 73 F6.2 deg Az Azimuth angle (measured through west from north) 75 I1 --- Nobs Number of observations -------------------------------------------------------------------------------- Note (1): Identifier: if it is listed by Ciardullo et al. (1989, Cat. J/ApJ/339/53), their identifier is used (of the form PNNN, Ford M 31 NNN in Simbad), otherwise it has an identifier from our imaging survey (PNfieldobject). Note (2): We have adopted the position of the nucleus listed in the NASA/IPAC Extragalactic Database (NED), close to that given by Crane, Dickel & Cowan (1992ApJ...390L...9C 1992ApJ...390L...9C). We assume a major axis position angle of 38.1°. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 19-Oct-2006
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