NGC 7036

0.14 UTI

0.0

C_N

0.06

C_dens

0.12

C_C3

0.25

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 24

Radius (P>50% members) 6.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.12 Very low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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NGC 7036 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, well below the mid-plane, affected by low extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~5.03 kpc) differs significantly from the median photometric distance (~1.19 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Low extinction Low mass Old

Cantat-Gaudin et al. (2020)
Flagged as non-existent; Gaia DR2 data show no coherent kinematic group despite proposed members. More details in Appendix A of the article.

Data

🔍 Search references for NGC 7036 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	–	317.495	15.519	0.199	-3.334	-5.641	-33.245
Angelo et al.	2019	317.492	15.514	–	–	–	–
Loktin & Popova	2017	317.505	15.517	–	1.44	-5.68	–
van den Bergh	2006	317.508	15.518	–	–	–	–
Dias et al.	2002	317.508	15.517	–	1.44	-5.68	–

💡 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
Angelo et al.	2019	1.46	–	–	2240	–	15	–	–
Loktin & Popova	2017	1.38	0.06	–	2163	–	–	–	–
van den Bergh	2006	1.00	0.31	–	3162	–	–	–	–
Dias et al.	2002	1.00	0.31	–	3162	–	–	–	–

Visualization

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