HSC 1413

0.49 UTI

0.47

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 47

Radius (P>50% members) 1.4 [arcmin]

C_N 0.47 Poorly 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 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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HSC 1413 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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.

Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1413 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	–	90.255	32.009	0.18	0.914	-1.098	10.936
Hunt & Reffert	2024	90.246	32.006	0.183	0.895	-1.086	10.767
Cavallo et al.	2024	90.259	32.033	0.176	–	–	–
Hunt & Reffert	2023	90.246	32.006	0.183	0.895	-1.086	10.767

💡 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
Hunt & Reffert	2024	–	–	–	–	–	763*	–	–
Cavallo et al.	2024	4.37	2.13	–	324	0.130	–	–	–
Hunt & Reffert	2023	5.00	2.15	2.10	379	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3290	83.0	90.25	32.01	0.17	0.93	-1.12	10.94	0.04

💡 Note: The % column shows the percentage of members that HSC 1413 shares with each listed object.

Visualization

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