NGC 2413

(MWSC 1262)

0.25 UTI

0.0

C_N

0.05

C_dens

0.12

C_C3

0.55

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 17

Radius (P>50% members) 7.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.12 Very low quality
C_lit 0.55 Moderately studied
C_dup 1.0 Unique

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

Overview

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NGC 2413 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.61 kpc) differs significantly from the median photometric distance (~0.60 kpc).

Close Low extinction Intermediate age

Dias et al. (2002)
Asterism (Archinal, B. A. & Hynes, S. J. 2003)

Data

🔍 Search references for NGC 2413 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	–	113.331	-13.112	0.277	-1.371	0.484	–
Just et al.	2023	113.259	-12.988	–	–	–	–
Bica et al.	2019	113.31	-13.097	–	–	–	–
Loktin & Popova	2017	113.28	-13.399	–	0.773	-0.162	–
Kharchenko et al.	2016	113.259	-12.988	–	–	–	–
Dias et al.	2014	113.279	-13.4	–	-2.35	2.13	–
Kharchenko et al.	2013	113.265	-12.99	–	-0.47	1.61	–
Piskunov et al.	2008	113.275	-13.036	–	–	–	–
Kharchenko et al.	2005	113.28	-13.04	–	-2.01	0.99	–
Dias et al.	2002	113.279	-13.4	–	-2.35	2.13	–

💡 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	–	–	–	452	–	97	–	–
Loktin & Popova	2017	0.76	0.46	–	377	–	–	–	–
Kharchenko et al.	2016	1.34	0.13	–	452	–	–	–	–
Kharchenko et al.	2013	1.34	0.13	–	452	–	–	–	–
Piskunov et al.	2008	0.44	0.12	–	288	–	–	–	–
Kharchenko et al.	2005	0.44	0.12	–	288	–	–	–	–
Dias et al.	2002	0.44	0.12	–	288	–	–	–	–

Visualization

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