XDOCC 05

0.45 UTI

0.52

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 54

Radius (P>50% members) 6.4 [arcmin]

C_N 0.52 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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XDOCC 05 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for XDOCC 05 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	–	121.76	-29.888	0.6	-3.619	3.604	35.866
Jaehnig et al.	2021	121.754	-29.901	0.598	-3.656	3.562	–

💡 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
Piatti et al.	2023	–	–	–	54	0.170	188	0.22	–
Jaehnig et al.	2021	1.64*	0.24	–	152	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0433	63.0	121.79	-29.89	0.6	-3.61	3.61	33.39	0.0
HSC 1995	46.3	121.76	-29.9	0.6	-3.62	3.6	33.39	0.0

💡 Note: The % column shows the percentage of members that XDOCC 05 shares with each listed object.

Visualization

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