ASCC 76

(MWSC 2171)

0.25 UTI

0.0

C_N

0.01

C_dens

0.12

C_C3

0.56

C_lit

1.0

C_dup

N₅₀ (P>50% members) 13

Stellar density (N₅₀/rad) 0.0 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.12 Very low quality
C_lit 0.56 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

ASCC 76 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~6.80 kpc) differs significantly from the median photometric distance (~0.60 kpc).

Close Low extinction Young

Data

🔍 Search references for ASCC 76 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	208.044	-66.385	0.147	-6.915	-2.932	-78.521
Just et al.	2023	208.046	-66.402	–	–	–	–
Bica et al.	2019	208.072	-66.395	–	–	–	–
Kharchenko et al.	2016	208.046	-66.402	–	–	–	–
Dias et al.	2014	208.067	-66.4	–	-3.36	-6.4	–
Kharchenko et al.	2013	208.057	-66.405	–	-4.25	-3.8	-14.0
Gozha et al.	2012	208.067	-66.4	–	–	–	–
Piskunov et al.	2008	208.048	-66.397	–	–	–	–
Kharchenko et al.	2007	208.06	-66.4	–	0.35	–	-14.0
Kharchenko et al.	2005	208.06	-66.4	–	-4.12	-3.34	-14.0
Dias et al.	2002	208.067	-66.4	–	-4.12	-3.34	-19.9

💡 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–	0.6	0.84	–	28	–	172	–	–
Just et al.	2023	–	–	–	56	–	135	–	–
Kharchenko et al.	2016	1.02	1.42	–	56	–	–	–	–
Kharchenko et al.	2013	1.02	1.42	–	56	–	–	–	–
Gozha et al.	2012	0.60	–	–	28	–	209	–	–
Piskunov et al.	2008	0.60	0.84	–	28	–	–	–	–
Kharchenko et al.	2005	0.60	0.84	–	28	–	–	–	–
Dias et al.	2002	0.60	0.84	–	28	–	–	–	–

Visualization

ℹ️