BDSB 97
(BDS2003 97)
0.18
UTI
0.3
CN
1.0
Cdens
0.38
CC3
0.0
Clit
0.53
Cdup
Nm (P>50%)
30
Core radius and density
0.5 [pc], 6.4 [pc-2]
- CN 0.3 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.53 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
BDSB 97 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close 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.
Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue. 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 | 260.005 | -35.958 | 0.593 | -0.294 | -2.237 | 71.955 |
| Morales et al. | 2013 | 260.012 | -35.972 | â | â | â | â |
| Bica et al. | 2003 | 260.013 | -35.966 | 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 | 1.74 | â | â | â | â | â | â | â |
| Morales et al. | 2013 | 1.74 | â | â | â | â | â | â | â |
Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: possibly associated submm emission surrounding the cluster, presence of emission related to PAH or warm dust.
Bica et al. (2003)
Classified as stellar group (IRGr).