Stock 13

(MWSC 1921)

Click to load Aladin Lite
0.78 UTI
0.64
CN
0.5
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 77
Radius (P>50% members) 6.2 [arcmin]
  • CN 0.64 Moderately populated
  • Cdens 0.5 Moderately dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
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 very 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
ℹī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 1101* – –
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* – – – – – – –
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* – –
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 – – – –

(*): Indicates that this parameter is assigned more than one value 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
ℹī¸
Stock 13 UCC
Stock 13 HUNT23
Galactocentric position diagram