J/A+A/586/A102      UCDs in the halo of NGC1399                  (Voggel+, 2016)

Globular cluster clustering and tidal features around ultra-compact dwarf galaxies in the halo of NGC 1399. Voggel K., Hilker M., Richtler T. <Astron. Astrophys., 586, A102-102 (2016)> =2016A&A...586A.102V 2016A&A...586A.102V (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, nearby ; Associations, stellar ; Clusters, globular Keywords: galaxies: clusters: individual: NGC 1399 - galaxies: dwarf - galaxies: fundamental parameters - galaxies: nuclei - galaxies: star clusters: general Abstract: We present a novel approach to constrain the formation channels of ultra-compact dwarf galaxies (UCDs). They most probably are an inhomogeneous class of objects, composed of remnants of tidally stripped dwarf elliptical galaxies and star clusters that occupy the high mass end of the globular cluster luminosity function. We use three methods to unravel their nature: 1) we analyzed their surface brightness profiles; 2) we carried out a direct search for tidal features around UCDs; and 3) we compared the spatial distribution of GCs and UCDs in the halo of their host galaxy. Based on FORS2 observations under excellent seeing conditions, we studied the detailed structural composition of a large sample of 97 UCDs in the halo of NGC1399, the central galaxy of the Fornax cluster, by analyzing their surface brightness profiles. We found that 13 of the UCDs were resolved above the resolution limit of 23pc and we derived their structural parameters fitting a single Sersic function. When decomposing their profiles into composite King and Sersic profiles, we find evidence for faint stellar envelopes at µ≃26mag/arcsec2, surrounding the UCDs up to an extension of 90pc in radius. We also show new evidence for faint asymmetric structures and tidal tail-like features surrounding several of these UCDs, a possible tracer of their origin and assembly history within their host galaxy halos. In particular, we present evidence for the first discovery of a significant tidal tail with an extension of ∼350pc around UCD-FORS2. Finally, we studied the local overdensities in the spatial distribution of globular clusters within the halo of NGC1399 out to 110kpc to see if they are related to the positions of the UCDs. We found a local overabundance of globular clusters on a scale of ≤1kpc around UCDs, when we compared it to the distribution of globulars from the host galaxy. This effect is strongest for the metal-poor blue GCs. We discuss how likely it is that these clustered globulars were originally associated with the UCD, either as globular cluster systems of a nucleated dwarf galaxy that was stripped down to its nucleus, or as a surviving member of a merged super star cluster complex. Description: To study UCDs within the Fornax cluster, we used data from ESO program 076.B-0520 (PI:Richtler). The imaging data were taken in the nights October 9th and 10th, 2005, with the high-resolution collimator mode of FORS2, which is mounted on UT1 of the Very Large Telescope (VLT). Three separate fields were observed in the R-band. Fields 1 and 2 with 3x800s exposure time each and field 3 with 5x800s. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 96 13 Results from the Sersic fits for those 13 UCDs that have half-light radii larger than the resolution limit of 23 pc tablea1.dat 89 21 UCD and companion properties of all 19 objects for which a faint point source was found within r<300pc (see Fig. 9) tablea2.dat 63 71 UCDs from the original sample of 97 in the FORS fields, which are not yet listed in Table 1 or as a companion hosting UCD in Table A.1 -------------------------------------------------------------------------------- See also: J/A+A/383/823 : Radial velocities of UCOs in Fornax (Mieske+, 2002) J/AJ/127/2114 : Globular clusters around NGC 1399 (Dirsch+, 2004) J/A+A/418/445 : FCOS Ultra Compact Dwarf galaxies radial vel. (Mieske+ 2004) J/A+A/513/A52 : Velocities of NGC 1399 globular clusters (Schuberth+, 2010) J/MNRAS/382/1342 : Compact stellar systems around NGC 1399 (Firth+, 2007) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- --- [UCD-FORS -] 10- 11 I2 --- UCD-FORS UCD-FORS number 13- 18 A6 --- AName Alternative name (G1) 20 A1 --- n_AName [abc] Note on AName (1) 23 I1 h RAh Right ascension (J2000) 25- 26 I2 min RAm Right ascension (J2000) 28- 32 F5.2 s RAs Right ascension (J2000) 34 A1 --- DE- Declination sign (J2000) 35- 36 I2 deg DEd Declination (J2000) 38- 39 I2 arcmin DEm Declination (J2000) 41- 44 F4.1 arcsec DEs Declination (J2000) 46- 50 F5.2 mag Vmag UCD V magnitude 52- 56 F5.3 mag e_Vmag rms uncertainty on Vmag 58- 62 F5.2 pc Reff Effective temperature 64- 67 F4.2 pc e_Reff rms uncertainty on Reff (2) 69- 72 F4.2 --- n Sersic index 74- 77 F4.2 --- e_n rms uncertainty on n (2) 79- 82 F4.2 mag V-I UCD V-I colour index (3) 84- 87 F4.2 mag e_V-I rms uncertainty on V-I 89- 92 I4 km/s RV Radial velocity (3) 94- 96 I3 km/s e_RV rms uncertainty on RV -------------------------------------------------------------------------------- Note (1): Some of these objects were also presented in Richtler et al. (2008A&A...478L..23R 2008A&A...478L..23R) with the following names: a = 78:12, [DRG2004] 78:12 in Simbad b = 91:93, [DRG2004] 91:93 in Simbad c = 90:12, [DRG2004] 90:12 in Simbad Note (2): The provided errors on Reff and n are those given by GALFIT, which should be taken with caution because close to the resolution limit these errors might be underestimated. Note (3): The (V-I) colors and radial velocities are taken from the respective original samples. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Ref Reference used in Fig. 9 3- 10 A8 --- --- [UCD-FORS -] 12- 13 I2 --- UCD-FORS UCD-FORS number 15- 20 A6 --- AName Alternative name 23 I1 h RAh Right ascension (J2000) 25- 26 I2 min RAm Right ascension (J2000) 28- 32 F5.2 s RAs Right ascension (J2000) 34 A1 --- DE- Declination sign (J2000) 35- 36 I2 deg DEd Declination (J2000) 38- 39 I2 arcmin DEm Declination (J2000) 41- 44 F4.1 arcsec DEs Declination (J2000) 46- 50 F5.2 mag Vmag UCD V magnitude 52- 55 F4.2 mag V-I UCD V-I colour index 57- 61 F5.2 mag Vcomp V magnitude of the possible companion 63- 65 I3 pc Distc Distance of the companion to the UCD 67- 71 F5.2 kpc DisttN Distance of the UCD to the center of NCG 1399 73- 75 I3 pc r Tidal radius (1) 77- 80 F4.2 --- Distc/r Fraction between Distc/r (2) 82- 85 I4 km/s RV Radial Velocity 87- 89 I3 km/s e_RV rms uncertainty on RV -------------------------------------------------------------------------------- Note (1): estimate of the tidal radius of this UCD for it's specific position using the formula given in 8. Note (2): If this fraction is smaller than 1.0 the companion lies within the tidal radius of the UCD host object, which is the case for 16 of our 19 UCDs. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- --- [UCD-FORS -] 10- 11 I2 --- UCD-FORS UCD-FORS number 13- 18 A6 --- AName Alternative name (G1) 21 I1 h RAh Right ascension (J2000) 23- 24 I2 min RAm Right ascension (J2000) 26- 30 F5.2 s RAs Right ascension (J2000) 32 A1 --- DE- Declination sign (J2000) 33- 34 I2 deg DEd Declination (J2000) 36- 37 I2 arcmin DEm Declination (J2000) 39- 42 F4.1 arcsec DEs Declination (J2000) 44- 48 F5.2 mag Vmag UCD V magnitude 50- 53 F4.2 mag e_Vmag rms uncertainty on Vmag 55- 58 F4.2 mag V-I UCD V-I colour index 60- 63 F4.2 mag e_V-I rms uncertainty on V-I -------------------------------------------------------------------------------- Global notes: Note (G1): The alternative object names from the literature are from the following sources: UCDx = Firth et al. (2007, Cat. J/MNRAS/382/1342) [DJG2000] UCO XX in Simbad X_xxx = Mieske et al. (2002, Cat. J/A+A/383/823 & 2004, Cat. J/A+A/418/445 FCOS F-NNNN in Simbad Yxxx = Richtler et al. (2008A&A...478L..23R 2008A&A...478L..23R), [MHB2008] Yxxx in Simbad or from Schuberth et al. (2010, Cat. J/A+A/513/A52), [SRH2010] NN NNN, [SRH2010] GS0N-M0N NNN in Simbad NN.NNN = Dirsch et al. (2014, Cat. J/AJ/127/2114), [DRG2004] NN:NNN in Simbad -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 22-Apr-2016
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