HXHWL 61

0.50 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 106

Stellar density (N₅₀/rad) 6.0 [N/pc²]

C3 classification AB

C_N 0.75 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

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

Overview

ℹ️

HXHWL 61 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate 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 Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for HXHWL 61 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	102.728	-9.974	0.476	-1.291	1.241	–
He et al.	2021	102.718	-9.968	0.5	-1.28	1.25	–

💡 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–	2.09	1.68	–	191	0.274	–	–	–
He et al.	2021	2.09	1.68	–	191	0.274	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2266	74.5	102.73	-9.99	0.48	-1.3	1.24	–	0.01
UBC 1354	60.4	102.73	-9.98	0.48	-1.3	1.24	–	0.0
CWWDL 13298	44.3	102.73	-9.98	0.47	-1.31	1.24	–	0.0

💡 Note: The % column shows the percentage of members that HXHWL 61 shares with each listed object.

Visualization

ℹ️