NGC 1996

(MWSC 608)

0.23 UTI

0.0

C_N

0.04

C_dens

0.12

C_C3

0.5

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 19

Radius (P>50% members) 5.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.12 Very low quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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NGC 1996 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 moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~6.65 kpc) differs significantly from the median photometric distance (~2.06 kpc).

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for NGC 1996 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	–	84.588	25.723	0.15	0.684	-0.916	-30.803
Just et al.	2023	84.539	25.75	–	–	–	–
Bica et al.	2019	84.581	25.873	–	–	–	–
Loktin & Popova	2017	84.54	25.75	–	0.098	-1.051	–
Kharchenko et al.	2016	84.539	25.75	–	–	–	–
Dias et al.	2014	84.542	25.817	–	-1.58	1.92	–
Kharchenko et al.	2013	84.547	25.75	–	0.14	-4.12	–
Piskunov et al.	2008	84.498	25.767	–	–	–	–
Kharchenko et al.	2005	84.51	25.77	–	0.58	-4.35	–

💡 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]	Bfr	BSS
Just et al.	2023	–	–	–	327	–	581	–	–
Loktin & Popova	2017	2.49	1.35	–	2239	–	–	–	–
Kharchenko et al.	2016	2.06	3.23	–	327	–	–	–	–
Kharchenko et al.	2013	2.06	3.23	–	327	–	–	–	–
Piskunov et al.	2008	1.40	0.46	–	282	–	–	–	–
Kharchenko et al.	2005	1.40	0.46	–	282	–	–	–	–

Visualization

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