Collinder 413

(NGC 6871; MWSC 3253; OCL 148; FoF 493)

0.96 UTI

0.81

C_N

1.0

C_dens

1.0

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 273

Stellar density (N₅₀/rad) 14.5 [N/pc²]

C3 classification AA

C_N 0.81 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

Collinder 413 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It is very well-studied in the literature.

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

Relatively close Moderate extinction Massive Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Collinder 413 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	301.511	35.764	0.515	-3.108	-6.458	0.538
Almeida et al.	2025	301.586	35.77	–	–	–	–
Zhang et al.	2024	301.49	35.776	–	–	–	–
Hunt & Reffert	2024	301.49	35.776	0.513	-3.092	-6.446	-0.99
Celli et al.	2024	301.548	35.765	–	–	–	–
Cavallo et al.	2024	301.593	35.753	0.514	–	–	–
Hunt & Reffert	2023	301.49	35.776	0.513	-3.092	-6.446	-0.99
Just et al.	2023	301.494	35.767	–	–	–	–
Jaehnig et al.	2021	301.518	35.769	0.544	-3.121	-6.426	–
Rain et al.	2021	301.548	35.765	0.514	-3.129	-6.437	–
Dias et al.	2021	301.586	35.77	0.516	-3.12	-6.444	–
Cantat-Gaudin et al.	2020	301.548	35.765	0.514	-3.129	-6.437	–
Cantat-Gaudin & Anders	2020	301.548	35.765	0.514	-3.129	-6.437	–
Liu & Pang	2019	301.488	35.791	0.522	-3.152	-6.444	–
Soubiran et al.	2018	301.548	35.765	–	–	–	4.38
Bica et al.	2019	301.497	35.77	–	–	–	–
Cantat-Gaudin et al.	2018	301.548	35.765	0.514	-3.129	-6.437	–
Loktin & Popova	2017	301.5	35.777	–	-2.676	-5.114	-10.5
Kharchenko et al.	2016	301.494	35.767	–	–	–	–
Dias et al.	2014	301.496	35.777	–	-3.26	-5.15	–
Kharchenko et al.	2013	301.5	35.77	–	-3.39	-6.82	-10.5
Gozha et al.	2012	301.496	35.777	–	–	–	–
Piskunov et al.	2008	301.486	35.776	–	–	–	–
Kharchenko et al.	2007	301.5	35.78	–	0.23	–	-10.54
Piskunov et al.	2007	301.486	35.776	–	–	–	–
van den Bergh	2006	301.5	35.783	–	–	–	–
Kharchenko et al.	2005	301.5	35.78	–	-3.65	-7.19	-10.54
Kharchenko et al.	2003	301.47	35.77	–	-3.68	-7.82	–
Chen et al.	2003	301.418	35.764	–	-3.23	-6.93	-7.7
Dias et al.	2002	301.496	35.777	–	-3.26	-5.15	-108.01
Dambis	1999	301.496	35.777	–	–	–	–

💡 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–	1.73	1.36	1.67	9	0.000	1148	–	0.0
Almeida et al.	2025	1.74	1.44	–	12	–	2423	–	–
Zhang et al.	2024	–	–	–	–	-0.050⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	1601⁽¹⁾	–	–
Celli et al.	2024	–	–	–	6	–	2822	–	–
Cavallo et al.	2024	1.81	1.43	–	8	0.000	–	–	–
Hunt & Reffert	2023	1.83	1.33	1.67	8	–	–	–	–
Just et al.	2023	–	–	–	10	–	863	–	–
Jaehnig et al.	2021	1.82⁽¹⁾	–	–	–	–	–	–	–
Rain et al.	2021	1.84	1.36	–	9	–	–	–	0
Dias et al.	2021	1.74	1.44	–	12	0.104	–	–	–
Cantat-Gaudin et al.	2020	1.72	1.19	–	5	–	–	–	–
Cantat-Gaudin & Anders	2020	1.84	–	–	–	–	–	–	–
Liu & Pang	2019	–	–	–	7	0.250	–	–	–
Soubiran et al.	2018	1.84	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	1.84	–	–	–	–	–	–	–
Loktin & Popova	2017	1.62	1.37	–	9	–	–	–	–
Kharchenko et al.	2016	1.79	1.29	–	10	–	–	–	–
Kharchenko et al.	2013	1.79	1.29	–	10	–	–	–	–
Gozha et al.	2012	1.57	–	–	9	-0.330	1148	–	–
Piskunov et al.	2008	1.57	1.36	–	10	–	499⁽¹⁾	–	–
Piskunov et al.	2007	1.57	1.36	–	10	–	116	–	–
van den Bergh	2006	1.57	1.36	–	9	–	–	–	–
Kharchenko et al.	2005	1.57	1.36	–	10	–	–	–	–
Kharchenko et al.	2003	1.57	1.36	–	–	–	–	–	–
Chen et al.	2003	1.57	–	–	0	–	–	–	–
Dias et al.	2002	1.57	1.37	–	9	–	–	–	–
Dambis	1999	1.51	1.39	–	10	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0102	6.6	301.71	35.64	0.53	-3.1	-6.61	-17.95	0.08

💡 Note: The % column shows the percentage of members that Collinder 413 shares with each listed object.

Visualization

ℹ️

1 2 3