Collinder 96

(MWSC 884)

0.36 UTI

0.33

C_N

0.31

C_dens

0.25

C_C3

0.45

C_lit

1.0

C_dup

N₅₀ (P>50% members) 33

Stellar density (N₅₀/rad) 1.5 [N/pc²]

C3 classification CC

C_N 0.33 Poorly populated
C_dens 0.31 Loose
C_C3 0.25 Low quality
C_lit 0.45 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Collinder 96 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.83 kpc) differs significantly from the median photometric distance (~1.06 kpc).

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Low mass Young

Data

🔍 Search references for Collinder 96 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–	97.588	2.863	0.353	-0.237	-0.928	40.24
Just et al.	2023	97.62	2.847	–	–	–	–
Jaehnig et al.	2021	97.617	2.842	0.124	0.13	0.383	–
Loktin & Popova	2017	97.575	2.867	–	0.44	-1.64	12.0
Kharchenko et al.	2016	97.62	2.847	–	–	–	–
Dias et al.	2014	97.575	2.867	–	-0.94	-4.2	12.0
Kharchenko et al.	2013	97.627	2.845	–	0.29	-3.09	12.0
van den Bergh	2006	97.575	2.867	–	–	–	–
Dias et al.	2002	97.575	2.867	–	0.44	-1.64	12.0

💡 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–	1.06	1.74	–	46	–	10	–	–
Just et al.	2023	–	–	–	63	–	10	–	–
Jaehnig et al.	2021	8.26⁽¹⁾	–	–	–	–	–	–	–
Loktin & Popova	2017	1.43	1.81	–	28	–	–	–	–
Kharchenko et al.	2016	1.06	1.74	–	63	–	–	–	–
Kharchenko et al.	2013	1.06	1.74	–	63	–	–	–	–
van den Bergh	2006	0.96	1.58	–	11	–	–	–	–
Dias et al.	2002	0.96	1.58	–	11	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 2655	36.4	97.66	2.99	0.37	-0.28	-0.96	–	0.02

💡 Note: The % column shows the percentage of members that Collinder 96 shares with each listed object.

Visualization

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