ASCC 80

(MWSC 2290)

0.33 UTI

0.0

C_N

0.01

C_dens

0.62

C_C3

0.5

C_lit

1.0

C_dup

N₅₀ (P>50% members) 14

Stellar density (N₅₀/rad) 0.1 [N/pc²]

C3 classification AC

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.62 Intermediate 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 80 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by low extinction. It is catalogued as a massive, young cluster (see Parameters). It is moderately studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~7.86 kpc) differs significantly from the median photometric distance (~1.50 kpc).

Relatively close Low extinction Massive Young

Data

🔍 Search references for ASCC 80 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–	231.212	-60.128	0.127	-4.917	-3.005	-8.185
Bica et al.	2019	231.143	-60.14	–	–	–	–
Kharchenko et al.	2016	231.174	-60.126	–	–	–	–
Dias et al.	2014	231.15	-60.14	–	-5.45	-3.32	–
Kharchenko et al.	2013	231.187	-60.128	–	-3.33	-5.03	-25.0
Gozha et al.	2012	231.15	-60.14	–	–	–	–
Piskunov et al.	2008	231.143	-60.14	–	–	–	–
Kharchenko et al.	2007	231.15	-60.14	–	0.25	–	-25.0
Kharchenko et al.	2005	231.15	-60.14	–	-2.6	-4.15	-25.0
Dias et al.	2002	231.15	-60.14	–	-5.45	-3.32	-25.0

💡 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–	1.5	0.53	–	85	–	2042	–	–
Kharchenko et al.	2016	1.28	1.23	–	237	–	–	–	–
Kharchenko et al.	2013	1.28	1.23	–	237	–	–	–	–
Gozha et al.	2012	1.50	–	–	85	–	2042	–	–
Piskunov et al.	2008	1.50	0.53	–	85	–	–	–	–
Kharchenko et al.	2005	1.50	0.53	–	85	–	–	–	–
Dias et al.	2002	1.50	0.53	–	85	–	–	–	–

Visualization

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