DBSB 95
(DBSB2003 95; DBSB 96; DBS2003 96; DBS2003 95)
0.24
UTI
0.39
CN
0.04
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Nm (P>50%)
39
Core radius and density
6.3 [pc], 0.2 [pc-2]
- CN 0.39 Poorly populated
- Cdens 0.04 Very loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 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 95 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate 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.
Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) 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 | 236.086 | -54.222 | 0.415 | -3.733 | -3.193 | -25.174 |
| Morales et al. | 2013 | 236.188 | -54.111 | â | â | â | â |
| Dutra et al. | 2003 | 236.187 | -54.097 | 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 | 2.67 | â | â | 2 | â | â | â | â |
| Morales et al. | 2013 | 2.67 | 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 emission related to PAH or warm dust.
Dutra et al. (2003)
Classified as infrared cluster (IRC).