XDOCC 03

0.07 UTI

0.39

C_N

0.29

C_dens

0.62

C_C3

0.0

C_lit

0.26

C_dup

C3 classification AC

Number of members (P>50%) 39

Radius (P>50% members) 15.3 [arcmin]

C_N 0.39 Poorly populated
C_dens 0.29 Loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.26 Possibly duplicate

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

Overview

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XDOCC 03 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Low extinction Near-solar metallicity Very young

Data

🔍 Search references for XDOCC 03 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	–	106.913	-13.034	0.86	-3.377	0.605	29.192
Jaehnig et al.	2021	107.01	-13.05	0.876	-3.319	0.546	–

💡 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	–	–	–	17	0.250	189	0.17	–
Jaehnig et al.	2021	1.14*	0.71	–	19	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FOF 2216	74.4	106.58	-12.81	0.87	-3.41	0.78	29.19	0.29
BDSB96	2.6	106.34	-12.34	0.86	-3.68	1.09	31.2	0.83
CMa08	2.6	107.43	-12.28	0.86	-3.15	0.88	26.44	0.5

💡 Note: The % column shows the percentage of members that XDOCC 03 shares with each listed object.

Visualization

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