1996A&A...310..715C


Query : 1996A&A...310..715C

1996A&A...310..715C - Astronomy and Astrophysics, volume 310715-721 (1996/6-3)

The Tucana dwarf Galaxy.

CASTELLANI M., MARCONI G. and BUONANNO R.

Abstract (from CDS):

We present deep CCD photometry for the dwarf galaxy in Tucana (l=323, b=-47.4). The data indicate that the galaxy is dominated by an intermediate/old stellar population with metallicity similar to that of the galactic globular clusters NGC 6752 and NGC 7089 (M2) (we find [Fe/H]≃-1.56). The distance modulus we derived, (m-M)V≃24.72±0.2, makes clear that this galaxy belongs to the Local Group. Tucana is clearly different from other dwarf galaxies, such as Leo I (Lee et al. 1993b), or Phoenix (Ortolani and Gratton 1988), because there is no evidence of a young stellar population (t≤5Gyrs) We suggest that the Tucana Galaxy is a genuine dwarf spheroidal in which no recent burst of star formation occurred.

Abstract Copyright: ∼

Journal keyword(s): stars: HR-diagrams - stars: luminosity functions - galaxies: elliptical - galaxies: stellar content - galaxies: individual: Tucana dwarf

VizieR on-line data: <Available at CDS (J/A+A/310/715): tucana.dat>

Nomenclature: Table 2: [CMB96] NNN (Nos 1-940).

Simbad objects: 12

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Number of rows : 12
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 104 GlC 00 24 05.359 -72 04 53.20     4.09     ~ 4158 0
2 NAME Phoenix Dwarf Galaxy Sy1 01 51 06.3 -44 26 41   13.48 13.2 12.69   ~ 575 2
3 NGC 1851 GlC 05 14 06.76 -40 02 47.6           ~ 1529 0
4 ESO 206-20A G 06 41 36.7 -50 57 58   22.14 11.0 19.47   ~ 1190 0
5 Z 64-73 G 10 08 28.12 +12 18 23.4   11.3 10.0     ~ 1284 1
6 NGC 6397 GlC 17 40 42.09 -53 40 27.6     5.17     ~ 2103 0
7 NGC 6752 GlC 19 10 52.11 -59 59 04.4           ~ 2121 0
8 MCG-02-53-003 G 20 46 51.7 -12 50 54 15.75 15.18 14.83 14.46   ~ 470 1
9 M 15 GlC 21 29 58.33 +12 10 01.2           ~ 3274 0
10 M 2 GlC 21 33 27.02 -00 49 23.7     6.25     ~ 1114 1
11 NAME Tuc Galaxy G 22 41 49.6 -64 25 10   15.7 15.2     ~ 324 0
12 Z 431-72 G 23 28 35.2 +14 44 35 13.85 13.16 12.52     ~ 499 1

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