DBSB 130
(DBS2003 130)
0.13
UTI
0.0
CN
0.05
Cdens
0.75
CC3
0.0
Clit
0.84
Cdup
Stellar density (N50/rad)
0.2 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.05 Very loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.84 Very likely unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
DBSB 130 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large* distance, near the mid-plane. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.
(*): The parallax distance estimate (~6.50 kpc) differs significantly from the median photometric distance (~3.80 kpc).
Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.84) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 198.123 | -62.765 | 0.154 | -7.284 | -0.654 | -12.55 |
| Morales et al. | 2013 | 197.975 | -62.784 | 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 | 3.8 | â | â | 2 | â | â | â | â |
| Morales et al. | 2013 | 3.80 | â | â | 2 | â | â | â | â |
Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of an IR bubble.