DBSB 92

(MWSC 2266)

0.09 UTI

0.0

C_N

0.06

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 12

Radius (P>50% members) 7.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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DBSB 92 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~2.97 kpc) differs significantly from the median photometric distance (~1.96 kpc).

⚠️ 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 Young

Data

🔍 Search references for DBSB 92 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	–	225.833	-57.559	0.337	-5.313	-3.729	8.798
Just et al.	2023	225.888	-57.678	–	–	–	–
Kharchenko et al.	2016	225.888	-57.678	–	–	–	–
Kharchenko et al.	2013	225.9	-57.68	–	-7.41	-2.42	–

💡 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]	Bfr	BSS
Just et al.	2023	–	–	–	25	–	140	–	–
Kharchenko et al.	2016	1.96	3.23	–	25	–	–	–	–
Kharchenko et al.	2013	1.96	3.23	–	25	–	–	–	–

Visualization

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