FoF 2036

(LP 2036)

0.27 UTI

0.42

C_N

0.18

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 42

Radius (P>50% members) 4.9 [arcmin]

C_N 0.42 Poorly populated
C_dens 0.18 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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FoF 2036 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

Data

🔍 Search references for FoF 2036 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	–	81.262	40.934	0.211	0.209	-0.253	8.925
Almeida et al.	2025	81.271	40.951	–	–	–	–
He et al.	2023	81.245	40.974	0.2	0.162	-0.253	-9.0
Dias et al.	2021	81.271	40.951	0.217	0.425	-0.251	-25.058

💡 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
Almeida et al.	2025	4.12	1.98	–	27	–	581	–	–
He et al.	2023	4.79	2.10	–	50	–	–	–	–
Dias et al.	2021	4.12	1.98	–	27	-0.205	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1309	47.6	81.29	40.93	0.2	0.17	-0.26	–	0.05

💡 Note: The % column shows the percentage of members that FoF 2036 shares with each listed object.

Visualization

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