UBC 606

0.09 UTI

0.0

C_N

0.02

C_dens

0.75

C_C3

0.0

C_lit

0.6

C_dup

C3 classification AB

Number of members (P>50%) 11

Radius (P>50% members) 15.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.6 Likely unique

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

Overview

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UBC 606 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.

Data

🔍 Search references for UBC 606 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	–	37.623	57.273	0.411	-0.278	-1.134	–
Almeida et al.	2025	37.463	57.371	–	–	–	–
Dias et al.	2021	37.463	57.371	0.407	-0.287	-1.154	–

💡 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
Almeida et al.	2025	2.46	2.17	–	10	–	220	–	–
Dias et al.	2021	2.46	2.17	–	10	-0.127	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 192	40.0	37.05	57.16	0.4	-0.43	-1.15	-27.22	0.53
Collinder 28	24.0	38.34	57.55	0.42	-0.28	-1.1	-37.49	0.96

💡 Note: The % column shows the percentage of members that UBC 606 shares with each listed object.

Visualization

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