J/A+A/429/819       Photometry in elliptical galaxies. II.   (Michard+, 2005)

Peculiarities and populations in elliptical galaxies. II. Visual-near IR colours as population indices. Michard R. <Astron. Astrophys., 429, 819-823 (2005)> =2005A&A...429..819M 2005A&A...429..819M (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, photometry Keywords: galaxies: elliptical and lenticulars, CD - galaxies: photometry Abstract: As a complement to the data collected and discussed in Paper I of this series (Michard & Prugniel, 2004, J/A+A/423/833) 2MASS near-IR images have been used, in connection with available V-light aperture photometry to derive the colours V-J, V-K, J-H and J-K within the effective aperture Ae: nearly the same complete sample of 110 E-type galaxies is treated. In Paper I these were classified, based on morphological criteria, into the "peculiar'' (or Pec) and "normal'' (or Nop) subsamples. The data included here supersede the previous catalog J/A+A/423/833. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file residual.dat 106 37 Residuals of colours- and line-indices of ellipticals in the Pec subsample, against the standard relations calculated for the Nop subsample between Indices and the central velocity dispersion (table7 of A&A, 423, 833 and table2 of this paper) table4.dat 150 117 Data compiled and derived for the full sample -------------------------------------------------------------------------------- See also: VII/184 : Survey of 108 E-S0 galaxies (Michard+, 1993-94) J/A+A/309/749 : Fundamental plane of early type galaxies (Prugniel+ 1996) J/A+AS/103/573 : UBVRI Photometry of bright southern galaxies (Poulain+ 1994) J/A+AS/104/179 : Surface photometry in Shapley-Ames galaxies (Goudfrooij+ 1994) J/ApJS/70/329 : IRAS flux densities for early-type galaxies (Knapp+ 1989) Byte-by-byte Description of file: residual.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name NGC, IC number 10- 13 F4.1 --- S2 Peculiarity index 16- 21 F6.3 mag D(U-B) U-B residual 23- 28 F6.3 mag D(B-V) B-V residual 30- 35 F6.3 mag D(B-R) ?=9.990 B-R residual 37- 42 F6.3 mag D(V-I) ?=9.990 V-I residual 44- 49 F6.3 mag D(Mg2) Mg2 index residual 51- 55 F5.2 0.1nm D(Hbeta) ?=9.99 Hbeta index residual 57- 61 F5.2 0.1nm D(<Fe>) ?=9.99 <Fe> index residual 63- 67 F5.2 0.1nm D(Mg_b) ?=9.99 Mgb index residual 69- 74 F6.3 mag D(V-J) ? V-J residual (2) 76- 81 F6.3 mag D(V-K) ? V-K residual (2) 83- 88 F6.3 mag D(J-H) ? J-H residual (2) 90- 95 F6.3 mag D(J-K) ? J-K residual (2) 97-102 F6.3 mag MIYPn Mean Index of Young Population 104-106 A3 --- Pop Family YP or NP (1) -------------------------------------------------------------------------------- Note (1): ":" stands for uncertain index. Note (2): NGC 1344 and NGC 3640 could not be measured in 2MASS. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name NGC or IC number 10- 14 F5.2 mag mu1 Distance modulus from Prugniel & Simien, 1996, Cat. J/A+A/309/749, hereafter PS96 16- 20 F5.2 mag mu2 Distance modulus from Tonry et al., 2001ApJ...546..681T 2001ApJ...546..681T 22- 26 F5.2 mag BT B total magnitude from PS96 28- 31 F4.2 [arcsec] logRe Adopted effective radius (derived from PS96) 33- 36 F4.2 --- eps Ellipticity near Re (1) 38- 43 F6.2 mag BMAG1 Absolute B magnitude from BT and Mu1 45- 50 F6.2 mag BMAG2 Absolute B magnitude from BT and Mu2 52- 55 F4.2 mag U-B Integrated U-B colour within Re (2) 57- 60 F4.2 mag B-V Integrated B-V colour within Re (2) 62- 65 F4.2 mag B-R Integrated B-R colour within Re (2) 67- 70 F4.2 mag V-I Integrated V-I colour within Re (2) 72- 75 F4.2 mag V-J Integrated V-J colour within Re (2) 77- 80 F4.2 mag V-K Integrated V-K colour within Re (2) 82- 85 F4.2 mag J-H Integrated J-H colour within Re (2) 87- 90 F4.2 mag J-K Integrated J-K colour within Re (2) 92- 96 F5.3 mag Mg2 Mg2 index from PS96 98-101 F4.2 0.1nm Hbeta Average Hβ index (3) 103 I1 --- W1 Number of Hbeta index sources 105-108 F4.2 0.1nm <Fe> Average <Fe> index (3) 110 I1 --- W2 Number of <Fe> index sources 112-115 F4.2 0.1nm Mgb Average Mgb index (3) 117 I1 --- W3 Number of Mgb index sources 119-121 I3 km/s sigma0 Central velocity dispersion 123-125 I3 km/s Vrot Maximum rotational velocity 127-130 I4 Jy F60um IRAS 60um flux normalized to Virgo distance (4) 132-135 I4 Jy F100um IRAS 100um flux normalized to Virgo distance (4) 137-140 F4.2 --- Dens Density of environment (unity in Virgo Cl.) 142-145 A4 --- Type Classification as boxy, disky, undeterminate 147-150 F4.1 --- S2 Peculiarity index (G1) -------------------------------------------------------------------------------- Note (1): Ellipticity is compiled from Goudfrooij et al., 1994, Cat. J/A+AS/104/179 and Michard & Marchal, 1994A&AS..105..481M 1994A&AS..105..481M, Cat. VII/184 Note (2): Colours are compiled from several sources with preference for Poulain & Nieto 1994, Cat. J/A+AS/103/573 Note (3): The line indices Hβ, <Fe>, Mg_b are compiled from severa l sources and averaged with a zero-point adjustment. Note (4): The IRAS fluxes at 60 and 100 microns are taken from Knapp et al., 1989, Cat. J/ApJS/70/329 and corrected to the Virgo Cluster distances. -------------------------------------------------------------------------------- Global Notes: Note (G1): The pecularity index S2 takes into account the following elements: - Discrete features classically recognized in possible post-mergers or in perturbed E-galaxies - Asymetries of the outer regions in E-galaxies - anomalous forms of the envelopes Objects with S2<1 are "normal", and the index varies from 0 to slightly above 10 for NGC 2865 and 3923, the most peculiar objects in the sample. -------------------------------------------------------------------------------- Acknowledgements: Raymond Michard, raymond.michard(at)obspm.fr References: Michard & Prugniel, Paper I 2004A&A...423..833M 2004A&A...423..833M, Cat. J/A+A/423/833
(End) Patricia Vannier [CDS] 18-Jan-2005
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