Dutra Bica 58

(MWSC 2677)

0.20 UTI

0.0

C_N

0.12

C_dens

0.38

C_C3

0.25

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 17

Radius (P>50% members) 8.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.12 Very loose
C_C3 0.38 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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Dutra Bica 58 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, very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.31 kpc) differs significantly from the median photometric distance (~1.18 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 Very young

Data

🔍 Search references for Dutra Bica 58 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	–	266.27	-28.885	0.434	-0.561	-1.615	-34.58
Just et al.	2023	266.259	-28.849	–	–	–	–
Kharchenko et al.	2016	266.259	-28.849	–	–	–	–
Kharchenko et al.	2013	266.268	-28.848	–	1.3	0.0	-15.5
Dias et al.	2002	266.25	-28.86	–	1.3	0.0	-15.5

💡 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	–	13	–	–
Kharchenko et al.	2016	1.18	6.13	–	1	–	–	–	–
Kharchenko et al.	2013	1.18	6.13	–	1	–	–	–	–
Dias et al.	2002	1.18	6.13	–	1	–	–	–	–

Visualization

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