HSC 595

0.52 UTI

0.59

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 68

Stellar density (N₅₀/rad) 35.7 [N/pc²]

C3 classification AA

C_N 0.59 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very 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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HSC 595 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, metal-rich, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Relatively close Very high extinction Massive Metal-rich Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 595 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–	306.592	36.447	0.337	-1.827	-2.796	-10.069
Hunt & Reffert	2024	306.593	36.449	0.342	-1.844	-2.822	-10.074
Cavallo et al.	2024	306.594	36.452	0.335	–	–	–
Hunt & Reffert	2023	306.593	36.449	0.342	-1.844	-2.822	-10.074

💡 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–	2.59	5.125	2.58	304	0.540	1257	–	–
Hunt & Reffert	2024	–	–	–	–	–	1257⁽¹⁾	–	–
Cavallo et al.	2024	2.61	5.04	–	380	0.540	–	–	–
Hunt & Reffert	2023	2.57	5.21	2.58	229	–	–	–	–

(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 2985	100.0	306.59	36.45	0.34	-1.8	-2.8	-10.07	0.18

💡 Note: The % column shows the percentage of members that HSC 595 shares with each listed object.

Visualization

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