ASCC 13

(MWSC 486)

0.86 UTI

0.61

C_N

0.95

C_dens

0.75

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 72

Stellar density (N₅₀/rad) 4.7 [N/pc²]

C3 classification AB

C_N 0.61 Moderately populated
C_dens 0.95 Very dense
C_C3 0.75 High quality
C_lit 1.0 Very 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 13 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.

Relatively close Low extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for ASCC 13 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–	78.207	44.377	0.895	-0.532	-1.797	-17.958
Li et al.	2025	78.255	44.417	0.898	-0.473	-1.743	–
Almeida et al.	2025	78.306	44.421	–	–	–	–
Zhang et al.	2024	78.221	44.365	–	–	–	–
Hunt & Reffert	2024	78.221	44.365	0.882	-0.548	-1.809	-17.423
Cavallo et al.	2024	78.141	44.424	0.888	–	–	–
Hunt & Reffert	2023	78.221	44.365	0.882	-0.548	-1.809	-17.423
Almeida et al.	2023	78.287	44.425	–	–	–	–
Just et al.	2023	78.439	44.596	–	–	–	–
He et al.	2022	78.206	44.358	0.893	-0.535	-1.817	–
Dias et al.	2021	78.306	44.421	0.899	-0.477	-1.737	–
Cantat-Gaudin et al.	2020	78.255	44.417	0.898	-0.473	-1.743	–
Cantat-Gaudin & Anders	2020	78.255	44.417	0.898	-0.473	-1.743	–
Bossini et al.	2019	78.255	44.417	–	–	–	–
Soubiran et al.	2018	78.255	44.417	–	–	–	32.37
Bica et al.	2019	78.328	44.58	–	–	–	–
Cantat-Gaudin et al.	2018	78.255	44.417	0.898	-0.473	-1.743	–
Kharchenko et al.	2016	78.439	44.596	–	–	–	–
Dias et al.	2014	78.329	44.58	–	1.99	-2.42	–
Kharchenko et al.	2013	78.45	44.595	–	-1.35	-4.3	-17.0
Gozha et al.	2012	78.329	44.58	–	–	–	–
Kharchenko et al.	2012	78.45	44.595	–	-1.34	-4.02	-16.95
Piskunov et al.	2008	78.328	44.58	–	–	–	–
Kharchenko et al.	2007	78.33	44.58	–	0.7	–	-16.95
Piskunov et al.	2007	78.328	44.58	–	–	–	–
Kharchenko et al.	2005	78.33	44.58	–	-0.75	-1.66	-7.3
Dias et al.	2002	78.329	44.58	–	-1.34	-4.02	-8.41

💡 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–	1.07	0.65	0.67	51	-0.098	713	0.62	–
Li et al.	2025	1.03	0.78	–	59	-0.148	–	–	–
Almeida et al.	2025	1.07	0.92	–	41	–	148	–	–
Zhang et al.	2024	–	–	–	–	-0.225⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	323⁽¹⁾	–	–
Cavallo et al.	2024	1.07	0.70	–	45	0.170	–	–	–
Hunt & Reffert	2023	1.07	0.62	0.67	88	–	–	–	–
Almeida et al.	2023	1.08	0.88	–	136	-0.120	576⁽¹⁾	0.62	–
Just et al.	2023	–	–	–	51	–	6516	–	–
He et al.	2022	–	0.80	–	45	–	–	–	–
Dias et al.	2021	1.07	0.92	–	41	-0.075	–	–	–
Cantat-Gaudin et al.	2020	1.12	0.70	–	32	–	–	–	–
Cantat-Gaudin & Anders	2020	1.08	–	–	–	–	–	–	–
Bossini et al.	2019	1.07	0.68	–	44	0.000	–	–	–
Soubiran et al.	2018	1.08	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	1.08	–	–	–	–	–	–	–
Kharchenko et al.	2016	0.80	0.62	–	51	–	–	–	–
Kharchenko et al.	2013	0.80	0.62	–	51	–	–	–	–
Gozha et al.	2012	0.80	–	–	51	–	2512	–	–
Kharchenko et al.	2012	0.80	0.62	–	51	–	–	–	–
Piskunov et al.	2008	0.80	0.62	–	51	–	1910⁽¹⁾	–	–
Piskunov et al.	2007	0.80	0.62	–	51	–	713	–	–
Kharchenko et al.	2005	0.80	0.62	–	51	–	–	–	–
Dias et al.	2002	0.80	0.62	–	51	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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