ASCC 116

(MWSC 3576)

0.25 UTI

0.0

C_N

0.04

C_dens

0.25

C_C3

0.48

C_lit

1.0

C_dup

N_m (P>50%) 17

Core radius and density 3.2 [pc], 0.2 [pc^-2]

C3 classification DB

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.25 Low quality
C_lit 0.48 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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ASCC 116 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as an extremely massive, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~5.17 kpc) differs significantly from the median photometric distance (~1.50 kpc).

Relatively close Moderate extinction Extremely massive Near-solar metallicity Young

Data

🔍 Search references for ASCC 116 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–	329.67	54.495	0.194	-2.874	-2.513	–
Just et al.	2023	329.62	54.487	–	–	–	–
Donor et al.	2020	329.625	54.49	–	-1.4	-2.03	-22.5
Bica et al.	2019	329.638	54.486	–	–	–	–
Dias et al.	2018	–	–	–	-3.8	-2.84	–
Dib et al.	2018	329.625	54.49	–	–	–	–
Sampedro et al.	2017	329.642	54.49	–	-3.6	-4.8	–
Joshi et al.	2016	329.625	54.49	–	–	–	–
Kharchenko et al.	2016	329.62	54.487	–	–	–	–
Dias et al.	2014	329.642	54.49	–	-3.44	-4.05	–
Kharchenko et al.	2013	329.625	54.49	–	-3.5	-4.5	-30.6
Gozha et al.	2012	329.642	54.49	–	–	–	–
Kharchenko et al.	2012	329.625	54.49	–	-3.5	-4.5	-30.6
Piskunov et al.	2008	329.638	54.486	–	–	–	–
Kharchenko et al.	2007	329.64	54.49	–	0.18	–	-30.6
Kharchenko et al.	2005	329.64	54.49	–	-3.51	-4.74	-30.6
Dias et al.	2002	329.642	54.49	–	-3.44	-4.05	-30.6

💡 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–	1.5	1.61	–	89	-0.130	16982	–	–
Just et al.	2023	–	–	–	89	–	81	–	–
Spina et al.	2022	–	–	–	–	-0.130	–	–	–
Donor et al.	2020	–	–	–	–	-0.130	–	–	–
Dib et al.	2018	1.50	–	–	89	–	–	–	–
Joshi et al.	2016	1.50	1.61	–	89	–	16982	–	–
Kharchenko et al.	2016	1.50	1.61	–	89	–	–	–	–
Kharchenko et al.	2013	1.50	1.61	–	89	–	–	–	–
Gozha et al.	2012	5.00	–	–	11	–	16982	–	–
Kharchenko et al.	2012	1.50	1.61	–	89	–	–	–	–
Piskunov et al.	2008	5.00	1.61	–	11	–	–	–	–
Kharchenko et al.	2005	5.00	1.61	–	11	–	–	–	–
Dias et al.	2002	5.00	1.61	–	11	–	–	–	–

Visualization

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