XDOCC 07

0.00 UTI

0.33

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 33

Stellar density (N₅₀/rad) 26.0 [N/pc²]

C3 classification AA

C_N 0.33 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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XDOCC 07 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for XDOCC 07 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–	159.441	-58.91	2.247	-14.372	0.916	9.484
Jaehnig et al.	2021	159.481	-58.723	2.281	-14.316	0.925	–

💡 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–	0.44	0.58	–	324	0.240	125	0.43	–
Piatti et al.	2023	–	–	–	575	0.240	125	0.43	–
Jaehnig et al.	2021	0.44⁽¹⁾	0.58	–	72	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
VDBH 99	100.0	159.52	-59.16	2.23	-14.47	0.99	8.58	1.0
HSC 2356	6.1	159.48	-59.03	2.05	-14.64	1.0	-11.52	0.0

💡 Note: The % column shows the percentage of members that XDOCC 07 shares with each listed object.

Visualization

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