DBSB 140

(DBS2003 140; MWSC 2276)

0.17 UTI

0.0

C_N

0.12

C_dens

0.25

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 18

Stellar density (N₅₀/rad) 0.6 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.12 Very loose
C_C3 0.25 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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DBSB 140 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by very high extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.95 kpc) differs significantly from the median photometric distance (~1.53 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 Very high extinction Low mass Young

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of emission related to PAH or warm dust.

Data

🔍 Search references for DBSB 140 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–	227.487	-58.352	0.339	-6.39	-4.55	-39.595
Just et al.	2023	227.501	-58.285	–	–	–	–
Kharchenko et al.	2016	227.501	-58.285	–	–	–	–
Kharchenko et al.	2013	227.512	-58.287	–	-6.22	-1.53	-9.7
Morales et al.	2013	227.492	-58.293	–	–	–	–

💡 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–	1.53	5.49	–	20	–	21	–	–
Just et al.	2023	–	–	–	20	–	21	–	–
Kharchenko et al.	2016	1.53	5.49	–	20	–	–	–	–
Kharchenko et al.	2013	1.53	5.49	–	20	–	–	–	–
Morales et al.	2013	12.14	–	–	–	–	–	–	–

Visualization

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