DBSB 165

(DBSB2003 165; DBS2003 165)

Click to load Aladin Lite
0.05 UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.0
Clit
0.96
Cdup
Core radius and density 5.3 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

â„šī¸
DBSB 165 is a sparse, very loose object of low 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 is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Morales et al. (2013)
Classified as morphological type 'EC1' (deeply embedded cluster). Morphological flag: cluster fully embedded, presence of emission related to PAH or warm dust.

Dutra et al. (2003)
Classified as infrared cluster (IRC).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 245.429 -50.422 0.401 -2.767 -4.112 -33.855
Morales et al. 2013 245.379 -50.418 – – – –
Dutra et al. 2003 245.377 -50.412 – – – –

💡 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 99999– 3.49 – – 3 – – – –
Morales et al. 2013 3.49 – – 3 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
BDB2003 G333.60-00.21 4.0 245.6 -50.12 0.35 -2.74 -4.01 -29.65 0.02
G333.6-0.2 4.0 245.61 -50.11 0.36 -2.73 -4.01 -14.28 0.03

💡 Note: The % column shows the percentage of members that DBSB 165 shares with each listed object.

Visualization

â„šī¸