DBSB 173

(DBSB2003 173; DBS2003 173)

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0.08 UTI
0.0
CN
0.02
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Core radius and density 4.8 [pc], 0.08 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
DBSB 173 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above 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 object shares a small percentage of members with 2 later reported entries. See table with shared members information.

âš 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.

Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: possibly associated submm emission surrounding the cluster, presence of an IR bubble and possible YSOs.

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 250.125 -45.608 0.249 -2.672 -3.988 151.021
Morales et al. 2013 250.072 -45.663 – – – –
Dutra et al. 2003 250.078 -45.662 – – – –

💡 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– 4.4 – – – – – – –
Morales et al. 2013 4.40 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 83 20.0 250.14 -45.47 0.22 -2.82 -4.13 -37.43 0.59
OC 0665 8.0 250.14 -45.47 0.19 -2.82 -4.12 29.9 0.0

💡 Note: The % column shows the percentage of members that DBSB 173 shares with each listed object.

Visualization

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