CMa08

0.50 UTI

0.76

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%) 132

Radius (P>50% members) 14.3 [arcmin]

C_N 0.76 Rich
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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CMa08 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near 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 object shares a moderate percentage of members with 5 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Very young

Data

🔍 Search references for CMa08 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	–	107.43	-12.276	0.856	-3.149	0.882	26.436
Santos-Silva et al.	2021	107.43	-12.3	0.84	-3.13	0.87	–

💡 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
Santos-Silva et al.	2021	1.14*	1.01*	–	18*	0.050*	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14345	40.2	107.43	-12.14	0.87	-3.2	0.92	22.81	0.01
CWWDL 14343	22.0	107.36	-12.04	0.85	-3.28	0.96	21.1	0.01
OC 0379	22.0	107.56	-12.45	0.84	-3.05	0.84	25.92	0.0
OC 0377	21.2	107.42	-12.04	0.85	-3.26	0.94	20.73	0.0
XDOCC 03	0.8	106.91	-13.03	0.86	-3.38	0.6	29.19	0.07

💡 Note: The % column shows the percentage of members that CMa08 shares with each listed object.

Visualization

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