DBSB 94

(DBSB2003 94; DBS2003 94; MWSC 2312)

0.12 UTI

0.0

C_N

0.16

C_dens

0.25

C_C3

0.1

C_lit

1.0

C_dup

N_m (P>50%) 17

Core radius and density 1.6 [pc], 0.8 [pc^-2]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.25 Low quality
C_lit 0.1 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 94 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Low mass Intermediate age

Morales et al. (2013)
Classified as morphological type 'EC1' (deeply embedded cluster). Morphological flag: cluster fully embedded, presence of an IR bubble.

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

Data

🔍 Search references for DBSB 94 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–	235.565	-53.955	0.486	-4.627	-3.835	-28.007
Just et al.	2023	235.563	-53.959	–	–	–	–
Kharchenko et al.	2016	235.563	-53.959	–	–	–	–
Kharchenko et al.	2013	235.575	-53.96	–	-3.7	-0.19	-42.4
Morales et al.	2013	235.575	-53.974	–	–	–	–
Dutra et al.	2003	235.572	-53.971	–	–	–	–

💡 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–	2.42	3.09	–	166	–	23	–	–
Just et al.	2023	–	–	–	166	–	23	–	–
Kharchenko et al.	2016	2.42	3.09	–	166	–	–	–	–
Kharchenko et al.	2013	2.42	3.09	–	166	–	–	–	–
Morales et al.	2013	2.67	–	–	–	–	–	–	–

Visualization

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