ASCC 14

(MWSC 507)

0.49 UTI

0.25

C_N

0.2

C_dens

0.38

C_C3

0.81

C_lit

1.0

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 1.0 [N/pc²]

C3 classification BC

C_N 0.25 Poorly populated
C_dens 0.2 Very loose
C_C3 0.38 Low quality
C_lit 0.81 Well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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ASCC 14 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.

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

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for ASCC 14 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–	80.091	35.217	0.921	-0.588	-3.647	-7.477
Zhang et al.	2024	80.004	35.229	–	–	–	–
Hunt & Reffert	2024	80.004	35.229	0.927	-0.564	-3.597	-15.069
Cavallo et al.	2024	80.126	35.228	0.927	–	–	–
Hunt & Reffert	2023	80.004	35.229	0.927	-0.564	-3.597	-15.069
Just et al.	2023	80.09	35.18	–	–	–	–
Bica et al.	2019	80.131	35.217	–	–	–	–
Kharchenko et al.	2016	80.09	35.18	–	–	–	–
Dias et al.	2014	80.129	35.22	–	-1.27	-4.76	–
Kharchenko et al.	2013	80.1	35.18	–	-0.03	-4.39	-16.9
Gozha et al.	2012	80.129	35.22	–	–	–	–
Kharchenko et al.	2012	80.1	35.18	–	-0.03	-4.39	-16.87
Piskunov et al.	2008	80.124	35.225	–	–	–	–
Kharchenko et al.	2007	80.13	35.22	–	0.22	–	-16.87
Kharchenko et al.	2005	80.13	35.22	–	-0.91	-5.98	-16.87
Dias et al.	2002	80.129	35.22	–	-1.27	-4.76	-16.87

💡 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–	1.1	0.68	0.83	339	-0.055	78	–	–
Zhang et al.	2024	–	–	–	–	-0.055⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	78⁽¹⁾	–	–
Cavallo et al.	2024	1.16	0.68	–	37	0.220	–	–	–
Hunt & Reffert	2023	0.99	0.68	0.83	49	–	–	–	–
Just et al.	2023	–	–	–	339	–	42	–	–
Kharchenko et al.	2016	1.10	1.15	–	339	–	–	–	–
Kharchenko et al.	2013	1.10	1.15	–	339	–	–	–	–
Gozha et al.	2012	1.10	–	–	407	–	240	–	–
Kharchenko et al.	2012	1.10	1.15	–	339	–	–	–	–
Piskunov et al.	2008	1.10	0.56	–	407	–	–	–	–
Kharchenko et al.	2005	1.10	0.56	–	407	–	–	–	–
Dias et al.	2002	1.10	0.56	–	407	-0.100	–	–	–

(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 1089	4.0	80.07	35.63	0.92	-0.24	-3.11	-14.17	0.15

💡 Note: The % column shows the percentage of members that ASCC 14 shares with each listed object.

Visualization

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