AH03 J1725 34.4
(BDSB 100; BDS2003 100)
0.39
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.16
Clit
0.69
Cdup
Stellar density (N50/rad)
60.2 [N/pc2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.16 Rarely studied
- Cdup 0.69 Likely unique
Overview
AH03 J1725 34.4 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 9 years.
(*): The parallax distance estimate (~1.79 kpc) differs significantly from the median photometric distance (~0.29 kpc).
Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 261.394 | -34.4 | 0.558 | -0.996 | -2.379 | 6.819 |
| Sampedro et al. | 2017 | 261.383 | -34.406 | -3.4 | 0.74 | â | â |
| Dias et al. | 2014 | 261.383 | -34.406 | â | -3.29 | -0.95 | â |
| Morales et al. | 2013 | 261.385 | -34.403 | â | â | â | â |
| Bukowiecki et al. | 2011 | 261.383 | -34.401 | â | â | â | â |
| Bica et al. | 2003 | 261.39 | -34.398 | â | â | â | â |
| Dias et al. | 2002 | 261.383 | -34.406 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.29 | 4.905 | â | 7 | â | 208 | â | â |
| Morales et al. | 2013 | 1.74 | â | â | â | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 208 | â | â |
| Bukowiecki et al. | 2011 | 0.29(1) | 4.83 | â | 7 | â | â | â | â |
| Dias et al. | 2002 | 0.29 | 4.98 | â | 7 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of an IR bubble.
Bica et al. (2003)
Classified as infrared cluster (IRC).