XDOCC 10

0.25 UTI

0.0

C_N

0.25

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 23

Radius (P>50% members) 7.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.25 Loose
C_C3 1.0 Very 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 10 is a sparse, loose object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high 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 3 later reported entries. See table with shared members information.

Relatively close High extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for XDOCC 10 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	–	305.525	37.238	0.501	-2.402	-5.264	53.948
Jaehnig et al.	2021	305.421	37.292	0.508	-2.387	-5.234	–

💡 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	–	–	–	708	0.400	655	0.29	–
Jaehnig et al.	2021	1.92*	3.97	–	23	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1101	72.0	305.72	37.19	0.49	-2.38	-5.32	46.61	0.44
CWWDL 1872	24.0	305.53	37.13	0.5	-2.43	-5.33	53.95	0.05
Theia 1975	20.0	305.52	37.04	0.5	-2.4	-5.36	53.95	0.06

💡 Note: The % column shows the percentage of members that XDOCC 10 shares with each listed object.

Visualization

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