Dutra Bica 33

(DB2000 33; MWSC 2679)

0.13 UTI

0.0

C_N

0.04

C_dens

0.38

C_C3

0.13

C_lit

1.0

C_dup

N_m (P>50%) 13

Core radius and density 2.5 [pc], 0.2 [pc^-2]

C3 classification CB

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.38 Low quality
C_lit 0.13 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Dutra Bica 33 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~4.03 kpc) differs significantly from the median photometric distance (~1.00 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 Very young

Dias et al. (2002)
Asterism (Dutra et al. 2003, A&A 408, 127); cat V3.5 (Jan 2016)

Data

🔍 Search references for Dutra Bica 33 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–	266.36	-26.738	0.248	-0.714	-2.923	-13.31
Bica et al.	2019	266.385	-26.7	–	–	–	–
Dib et al.	2018	266.37	-26.697	–	–	–	–
Joshi et al.	2016	266.37	-26.697	–	–	–	–
Kharchenko et al.	2016	266.361	-26.698	–	–	–	–
Kharchenko et al.	2013	266.37	-26.697	–	0.76	-2.41	–
Dutra & Bica	2000	266.385	-26.7	–	–	–	–

💡 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–	1.0	7.88	–	6	–	–	–	–
Dib et al.	2018	1.00	–	–	6	–	–	–	–
Joshi et al.	2016	1.00	7.88	–	6	–	–	–	–
Kharchenko et al.	2016	1.00	7.88	–	6	–	–	–	–
Kharchenko et al.	2013	1.00	7.88	–	6	–	–	–	–

Visualization

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