Stock 13

(MWSC 1921)

0.73 UTI

0.64

C_N

0.5

C_dens

0.75

C_C3

0.87

C_lit

1.0

C_dup

N₅₀ (P>50% members) 77

Stellar density (N₅₀/rad) 2.5 [N/pc²]

C3 classification AB

C_N 0.64 Moderately populated
C_dens 0.5 Moderately dense
C_C3 0.75 High quality
C_lit 0.87 Well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Stock 13 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is well-studied in the literature.

(*): The parallax distance estimate (~3.07 kpc) differs significantly from the median photometric distance (~1.58 kpc).

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

Relatively close Low extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Stock 13 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–	168.293	-58.885	0.326	-6.027	1.905	-13.118
Hunt & Reffert	2024	168.125	-58.779	0.322	-6.041	1.91	-8.503
Cavallo et al.	2024	168.304	-58.874	0.326	–	–	–
Hunt & Reffert	2023	168.125	-58.779	0.322	-6.041	1.91	-8.503
Just et al.	2023	168.239	-58.877	–	–	–	–
Jaehnig et al.	2021	168.282	-58.889	0.353	-6.022	1.828	–
Loktin & Popova	2017	168.27	-58.883	–	-5.49	-2.72	1.0
Kharchenko et al.	2016	168.239	-58.877	–	–	–	–
Dias et al.	2014	168.271	-58.883	–	-5.49	-2.72	–
Kharchenko et al.	2013	168.247	-58.88	–	-9.9	1.56	1.0
Gozha et al.	2012	168.271	-58.883	–	–	–	–
Piskunov et al.	2008	168.257	-58.876	–	–	–	–
Kharchenko et al.	2007	168.27	-58.88	–	0.23	–	1.0
Piskunov et al.	2007	168.257	-58.876	–	–	–	–
van den Bergh	2006	168.275	-58.883	–	–	–	–
Kharchenko et al.	2005	168.27	-58.88	–	-9.8	2.91	1.0
Kharchenko et al.	2003	168.27	-58.89	–	-9.16	2.89	–
Dias et al.	2002	168.271	-58.883	–	-5.49	-2.72	1.0
Dambis	1999	168.271	-58.883	–	–	–	–

💡 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–	1.58	0.68	1.46	17	-0.440	519	–	–
Hunt & Reffert	2024	–	–	–	–	–	1101⁽¹⁾	–	–
Cavallo et al.	2024	1.99	0.86	–	16	-0.440	–	–	–
Hunt & Reffert	2023	2.87	0.81	1.46	11	–	–	–	–
Just et al.	2023	–	–	–	23	–	303	–	–
Jaehnig et al.	2021	2.86⁽¹⁾	–	–	–	–	–	–	–
Loktin & Popova	2017	1.58	0.68	–	17	–	–	–	–
Kharchenko et al.	2016	1.58	0.69	–	23	–	–	–	–
Kharchenko et al.	2013	1.58	0.69	–	23	–	–	–	–
Gozha et al.	2012	1.58	–	–	17	–	1995	–	–
Piskunov et al.	2008	1.58	0.68	–	23	–	519⁽¹⁾	–	–
Piskunov et al.	2007	1.58	0.68	–	23	–	140	–	–
van den Bergh	2006	1.58	0.68	–	17	–	–	–	–
Kharchenko et al.	2005	1.58	0.68	–	23	–	–	–	–
Kharchenko et al.	2003	1.58	0.68	–	–	–	–	–	–
Dias et al.	2002	1.58	0.68	–	17	–	–	–	–
Dambis	1999	2.04	0.70	–	3	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 267	50.6	168.35	-58.94	0.32	-6.02	1.83	–	0.14

💡 Note: The % column shows the percentage of members that Stock 13 shares with each listed object.

Visualization

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