DBSB 134
(DBS2003 134)
0.13
UTI
0.0
CN
0.07
Cdens
0.75
CC3
0.0
Clit
0.8
Cdup
Stellar density (N50/rad)
0.3 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.07 Very loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.8 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 134 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 cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.
(*): The parallax distance estimate (~5.79 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=0.8) 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 | 198.38 | -62.725 | 0.173 | -6.986 | -0.604 | -31.819 |
| Morales et al. | 2013 | 198.592 | -62.744 | 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 | â | â | â | â | â |
| Morales et al. | 2013 | 3.80 | â | â | â | 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 and possible YSOs.