J/ApJS/141/61       Morphology of satellite galaxies          (Gutierrez+, 2002)

The properties of satellite galaxies in external systems. I. Morphology and structural parameters. Gutierrez C.M., Azzaro M., Prada F. <Astrophys. J. Suppl. Ser. 141, 61 (2002)> =2002ApJS..141...61G 2002ApJS..141...61G
ADC_Keywords: Galaxies, optical ; Morphology Keywords: galaxies: fundamental parameters - galaxies: general - galaxies: structure Abstract: We present the first results of an ongoing project to study the morphological, kinematical, dynamical, and chemical properties of satellite galaxies of external giant spiral galaxies. The sample of objects has been selected from the catalog by Zaritsky et al. (1993ApJ...405..464Z 1993ApJ...405..464Z). The paper analyzes the morphology and structural parameters of a subsample of 60 such objects. The satellites span a great variety of morphologies and surface brightness profiles. About two-thirds of the sample are spirals and irregulars, the remaining third being early-types. Some cases showing interaction between pairs of satellites are presented and briefly discussed. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 95 60 Morphology and Structural Parameters of Satellite Galaxies -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [ZSFW] 6- 11 A6 --- ZSFW Galaxy name (1) 13- 14 I2 h RAh Right ascension (J2000.0) (from Simbad) 16- 17 I2 min RAm Right ascension (J2000.0) (from Simbad) 19- 22 F4.1 s RAs Right ascension (J2000.0) (from Simbad) 24 A1 --- DE- Declination sign (J2000.0) (from Simbad) 25- 26 I2 deg DEd Declination (J2000.0) (from Simbad) 28- 29 I2 arcmin DEm Declination (J2000.0) (from Simbad) 31- 32 I2 arcsec DEs Declination (J2000.0) 34- 38 F5.1 mag BMAG Absolute B magnitude, from Zaritsky et al., 1997ApJ...478...39Z 1997ApJ...478...39Z 40- 42 I3 kpc Dist Projected distance between the satellite and the parent galaxy 44 A1 --- Filt [VRI] Filter used 46- 49 F4.1 arcsec re ? Radius of the bulge in arcsec (h0=0.75) 51- 53 F3.1 kpc re21 ? Radius of the bulge in kpc (h0=0.75) 55- 57 F3.1 --- n ? Sersic parameter of the bulge (3) 59- 62 F4.1 arcsec rd ? Length scale of the disk in arcsec 64- 66 F3.1 kpc rd2 ? Length scale of the disk in kpc 68- 71 F4.2 --- B/T ? Bulge to total luminosity ratio, computed from the structural parameters above 73- 95 A23 --- HType Morphological Hubble type (2) -------------------------------------------------------------------------------- Note (1): We wish to make the following remarks on some of the individual objects: 1. ZSFW N488c and ZSFW N2424b are examples of a low surface brightness galaxies without any structure. Other galaxies in the sample such as NGC 4030c also have low surface brightness, but in this case there are knots. 2. There are a few cases of spiral edge-on galaxies in which we were not able to determine the Hubble type and no satisfactory fit was found. In these cases we have classified them as S. 3. Many galaxies (∼25%) show signs of distortion, and at least in two cases interactions (see below). 4. ZSFW N488b and ZSFW N2775b are examples of spiral galaxies with very distorted disks. In the case of ZSFW N488b only the bulge was fitted. Note (2): For the great majority of the objects it was possible to determine their morphological type. The symbols * and ** quoted in some of the cases mean uncertain classification and signs of distortion/interaction, respectively. Note (3): the Sersic parameter n expressed the luminosity L being proportional to r(1/n) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) James Marcout, Patricia Bauer [CDS] 17-Sep-2002
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