DBSB 123

(DBS2003 123)

0.34 UTI

0.0

C_N

0.97

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 24

Stellar density (N₅₀/rad) 4.8 [N/pc²]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.97 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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DBSB 123 is a sparse, very dense object of high C3 quality. Its parallax locates it at a relatively close 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 large percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close Very young

Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: possibly associated submm emission surrounding the cluster.

Data

🔍 Search references for DBSB 123 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	259.269	-36.323	0.562	-0.201	-2.21	–
Morales et al.	2013	259.312	-36.338	–	–	–	–

💡 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]	B_frac	BSS
UCC	99999–	1.74	–	–	2	–	–	–	–
Morales et al.	2013	1.74	–	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
DBSB 122	96.0	259.25	-36.35	0.56	-0.16	-2.22	-76.6	0.46
HSC 2897	56.0	259.2	-36.36	0.56	-0.2	-2.22	-403.31	0.01

💡 Note: The % column shows the percentage of members that DBSB 123 shares with each listed object.

Visualization

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