CWNU 1136

0.35 UTI

0.59

C_N

0.39

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 68

Stellar density (N₅₀/rad) 1.9 [N/pc²]

C3 classification AB

C_N 0.59 Moderately populated
C_dens 0.39 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1136 is a moderately populated, loose object of 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 very young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 4 later reported entries. See table with shared members information.

Low extinction Very young

Data

🔍 Search references for CWNU 1136 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–	186.943	-60.634	9.216	-36.687	-12.148	12.268
He et al.	2022	187.592	-59.435	9.213	-36.298	-12.088	–

💡 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–	–	0.05	–	14	–	–	–	–
He et al.	2022	–	0.05	–	14	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 177	88.2	185.96	-63.25	9.36	-37.38	-11.21	12.41	0.44
OCSN 178	64.7	191.21	-57.65	8.99	-34.71	-14.46	11.89	0.47
HSC 2468	57.4	185.31	-56.63	9.04	-35.54	-11.74	12.65	0.24
HSC 2505	36.8	185.58	-64.05	9.33	-37.8	-10.73	12.41	0.0

💡 Note: The % column shows the percentage of members that CWNU 1136 shares with each listed object.

Visualization

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