DBSB 122

(DBSB2003 122; DBS2003 122)

0.33 UTI

0.53

C_N

0.36

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 56

Core radius and density 1.4 [pc], 1.8 [pc^-2]

C3 classification AB

C_N 0.53 Moderately populated
C_dens 0.36 Loose
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 122 is a moderately populated, loose object of high 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 object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close

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 stellar group (IRGr).

Data

🔍 Search references for DBSB 122 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–	259.247	-36.35	0.562	-0.159	-2.22	-76.597
Morales et al.	2013	259.258	-36.349	–	–	–	–
Dutra et al.	2003	259.259	-36.345	–	–	–	–

💡 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	–	–	–	–	–	–	–
Morales et al.	2013	1.74	–	–	–	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
DBSB 123	42.9	259.27	-36.32	0.56	-0.2	-2.21	–	0.22
HSC 2897	42.9	259.2	-36.36	0.56	-0.2	-2.22	-403.31	0.01

💡 Note: The % column shows the percentage of members that DBSB 122 shares with each listed object.

Visualization

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