ASCC 130

(MWSC 3768)

0.26 UTI

0.0

C_N

0.17

C_dens

0.12

C_C3

0.5

C_lit

1.0

C_dup

N₅₀ (P>50% members) 21

Stellar density (N₅₀/rad) 0.9 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.17 Very loose
C_C3 0.12 Very low quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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ASCC 130 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is moderately studied in the literature.

Distant Moderate extinction Very young

Data

🔍 Search references for ASCC 130 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–	358.228	62.446	0.311	-3.233	-1.321	-68.141
Just et al.	2023	358.17	62.445	–	–	–	–
Bica et al.	2019	358.203	62.444	–	–	–	–
Kharchenko et al.	2016	358.17	62.445	–	–	–	–
Dias et al.	2014	358.2	62.44	–	0.84	4.58	–
Kharchenko et al.	2013	358.177	62.448	–	-1.48	-1.35	–
Kharchenko et al.	2012	358.177	62.448	–	-1.48	-1.35	–
Piskunov et al.	2008	358.187	62.432	–	–	–	–
Kharchenko et al.	2005	358.2	62.44	–	-1.22	0.35	–
Dias et al.	2002	358.2	62.44	–	0.84	4.58	–

💡 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–	3.45	1.735	–	17	–	349	–	–
Just et al.	2023	–	–	–	17	–	349	–	–
Kharchenko et al.	2016	3.50	1.86	–	17	–	–	–	–
Kharchenko et al.	2013	3.50	1.86	–	17	–	–	–	–
Kharchenko et al.	2012	3.50	1.86	–	17	–	–	–	–
Piskunov et al.	2008	3.40	1.61	–	11	–	–	–	–
Kharchenko et al.	2005	3.40	1.61	–	11	–	–	–	–
Dias et al.	2002	3.40	1.61	–	11	–	–	–	–

Visualization

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