NGC 3036

(MWSC 1719; ESO 126 27)

0.24 UTI

0.0

C_N

0.07

C_dens

0.25

C_C3

0.45

C_lit

1.0

C_dup

N₅₀ (P>50% members) 17

Stellar density (N₅₀/rad) 0.3 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.07 Very loose
C_C3 0.25 Low quality
C_lit 0.45 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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NGC 3036 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, metal-poor, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.09 kpc) differs significantly from the median photometric distance (~1.20 kpc).

Relatively close Moderate extinction Low mass Metal-poor Intermediate age

Data

🔍 Search references for NGC 3036 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–	147.296	-62.624	0.324	-6.77	4.976	5.405
Just et al.	2023	147.311	-62.666	–	–	–	–
Bica et al.	2019	147.329	-62.663	–	–	–	–
Kharchenko et al.	2016	147.311	-62.666	–	–	–	–
Dias et al.	2014	147.317	-62.672	–	-4.47	2.09	–
Kharchenko et al.	2013	147.315	-62.67	–	-9.76	4.68	11.8
Piskunov et al.	2008	147.315	-62.67	–	–	–	–
Kharchenko et al.	2005	147.31	-62.67	–	-7.43	-1.25	–
Dias et al.	2002	147.317	-62.672	–	-4.47	2.09	11.78

💡 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–	1.2	1.24	–	692	-0.714	33	–	–
Just et al.	2023	–	–	–	977	–	33	–	–
Kharchenko et al.	2016	1.27	1.29	–	977	–	–	–	–
Kharchenko et al.	2013	1.27	1.29	–	977	-0.714	–	–	–
Piskunov et al.	2008	1.20	1.24	–	407	–	–	–	–
Kharchenko et al.	2005	1.20	1.24	–	407	–	–	–	–
Dias et al.	2002	1.20	1.24	–	407	-0.714	–	–	–

Visualization

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