DBSB 141

(MWSC 2297)

0.10 UTI

0.0

C_N

0.15

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 15

Radius (P>50% members) 5.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.15 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

ℹ️

DBSB 141 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 massive, very young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~2.67 kpc) differs significantly from the median photometric distance (~5.24 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.

Very distant Very high extinction Massive Very young

Data

🔍 Search references for DBSB 141 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	232.155	-56.377	0.374	-5.798	-4.49	-36.355
Just et al.	2023	232.136	-56.374	–	–	–	–
Kharchenko et al.	2016	232.136	-56.374	–	–	–	–
Kharchenko et al.	2013	232.147	-56.375	–	-2.72	-0.75	–

💡 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	–	–	–	1	–	3170	–	–
Kharchenko et al.	2016	5.24	6.78	–	1	–	–	–	–
Kharchenko et al.	2013	5.24	6.78	–	1	–	–	–	–

Visualization

ℹ️