ASCC 114

(MWSC 3542; FoF 2248)

0.96 UTI

0.79

C_N

1.0

C_dens

1.0

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 204

Stellar density (N₅₀/rad) 21.2 [N/pc²]

C3 classification AA

C_N 0.79 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very 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

ℹ️

ASCC 114 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, near 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 mass parameter (see Parameters). It is very well-studied in the literature.

Close Low extinction Near-solar metallicity Young

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

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for ASCC 114 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	324.99	53.975	1.069	-3.715	-3.462	-21.625
Li et al.	2025	324.99	53.997	1.066	-3.716	-3.421	–
Almeida et al.	2025	324.979	53.999	–	–	–	–
Alfonso et al.	2024	325.018	53.996	1.038	-3.698	-3.461	–
Hunt & Reffert	2024	325.063	53.99	1.06	-3.698	-3.475	-19.554
Cavallo et al.	2024	324.987	53.986	1.066	–	–	–
Hunt & Reffert	2023	325.063	53.99	1.06	-3.698	-3.475	-19.554
Almeida et al.	2023	324.997	53.972	–	–	–	–
Just et al.	2023	325.0	53.961	–	–	–	–
He et al.	2022	325.023	54.014	1.067	-3.704	-3.465	–
Dias et al.	2021	324.979	53.999	1.063	-3.754	-3.435	–
Cantat-Gaudin et al.	2020	324.99	53.997	1.066	-3.716	-3.421	–
Cantat-Gaudin & Anders	2020	324.99	53.997	1.066	-3.716	-3.421	–
Liu & Pang	2019	324.995	54.001	1.069	-3.718	-3.429	–
Bossini et al.	2019	324.99	53.997	–	–	–	–
Bica et al.	2019	325.006	53.968	–	–	–	–
Cantat-Gaudin et al.	2018	324.99	53.997	1.066	-3.716	-3.421	–
Kharchenko et al.	2016	325.0	53.961	–	–	–	–
Dias et al.	2014	325.004	53.97	–	-4.25	-4.52	–
Kharchenko et al.	2013	325.005	53.965	–	-3.7	-2.55	-22.0
Gozha et al.	2012	325.004	53.97	–	–	–	–
Kharchenko et al.	2012	325.005	53.965	–	-3.7	-2.55	-22.0
Piskunov et al.	2008	325.006	53.968	–	–	–	–
Kharchenko et al.	2007	325.0	53.97	–	0.16	–	-22.0
Kharchenko et al.	2005	325.0	53.97	–	-3.62	-3.38	-22.0
Dias et al.	2002	325.004	53.97	–	-4.25	-4.52	-22.0

💡 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–	0.89	0.92	1.7	56	0.034	429	0.68	–
Li et al.	2025	0.84	1.00	–	38	-0.041	–	–	–
Almeida et al.	2025	0.91	1.22	–	43	–	429	–	–
Alfonso et al.	2024	0.91	0.92	–	62	0.034	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	673⁽¹⁾	–	–
Cavallo et al.	2024	0.93	1.09	–	39	0.080	–	–	–
Hunt & Reffert	2023	0.89	1.06	1.70	33	–	–	–	–
Almeida et al.	2023	0.90	1.21	–	127	0.059	432⁽¹⁾	0.68	–
Just et al.	2023	–	–	–	56	–	8	–	–
He et al.	2022	–	1.30	–	32	–	–	–	–
Dias et al.	2021	0.91	1.22	–	43	0.035	–	–	–
Cantat-Gaudin et al.	2020	0.91	0.92	–	48	–	–	–	–
Cantat-Gaudin & Anders	2020	0.91	–	–	–	–	–	–	–
Liu & Pang	2019	–	–	–	32	-0.250	–	–	–
Bossini et al.	2019	0.89	0.90	–	56	0.000	–	–	–
Cantat-Gaudin et al.	2018	0.91	–	–	–	–	–	–	–
Kharchenko et al.	2016	0.59	0.81	–	56	–	–	–	–
Kharchenko et al.	2013	0.59	0.81	–	56	–	–	–	–
Gozha et al.	2012	0.55	–	–	56	–	11	–	–
Kharchenko et al.	2012	0.59	0.81	–	56	–	–	–	–
Piskunov et al.	2008	0.55	0.81	–	56	–	–	–	–
Kharchenko et al.	2005	0.55	0.81	–	56	–	–	–	–
Dias et al.	2002	0.55	0.81	–	56	–	–	–	–

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

Visualization

ℹ️

1 2 3