Dutra Bica 60

(MWSC 2657; DB2001 2; BDB 4; MWSC 2656)

0.18 UTI

0.0

C_N

0.01

C_dens

0.25

C_C3

0.31

C_lit

1.0

C_dup

C3 classification DB

Number of members (P>50%) 12

Radius (P>50% members) 10.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.25 Low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

ℹ️

Dutra Bica 60 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~6.82 kpc) differs significantly from the median photometric distance (~3.05 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.

Distant High extinction Old

Data

🔍 Search references for Dutra Bica 60 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	264.866	-23.701	0.147	-2.698	-5.312	6.316
Just et al.	2023	264.824	-23.659	–	–	–	–
Bica et al.	2019	264.832	-23.684	–	–	–	–
Kharchenko et al.	2016	264.824	-23.659	–	–	–	–
Kharchenko et al.	2013	264.832	-23.658	–	-5.44	-9.21	–
Dias et al.	2002	264.833	-23.683	–	-3.58	-3.89	–

💡 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	–	–	–	1585	–	96	–	–
Kharchenko et al.	2016	3.05	4.58	–	1585	–	–	–	–
Kharchenko et al.	2013	3.05	4.58	–	1585	–	–	–	–
Dias et al.	2002	3.05	4.58	–	1585	–	–	–	–

Visualization

ℹ️