Stock 17

(MWSC 3754)

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0.64 UTI
0.48
CN
0.34
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 48
Radius (P>50% members) 5.8 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 0.34 Loose
  • CC3 0.75 High quality
  • Clit 0.82 Well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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Stock 17 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is well-studied in the literature.

(*): The parallax distance estimate (~3.13 kpc) differs significantly from the median photometric distance (~2.40 kpc).

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

Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for Stock 17 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 – 355.966 62.16 0.32 -3.699 -1.56 –
Hunt & Reffert 2024 355.954 62.16 0.317 -3.639 -1.579 –
Celli et al. 2024 355.949 62.161 – – – –
Cavallo et al. 2024 356.3 62.084 0.317 – – –
Hunt & Reffert 2023 355.954 62.16 0.317 -3.639 -1.579 –
Just et al. 2023 355.938 62.162 – – – –
Cantat-Gaudin et al. 2020 355.949 62.161 0.309 -3.691 -1.525 –
Cantat-Gaudin & Anders 2020 355.949 62.161 0.309 -3.691 -1.525 –
Cantat-Gaudin et al. 2018 355.949 62.161 0.309 -3.691 -1.525 –
Loktin & Popova 2017 355.95 62.16 – -1.58 -2.55 -44.8
Kharchenko et al. 2016 355.938 62.162 – – – –
Kharchenko et al. 2013 355.947 62.165 – -2.05 -6.88 -44.8
Kharchenko et al. 2012 355.947 62.165 – -2.05 -7.0 -44.8
van den Bergh 2006 356.5 62.183 – – – –
Dias et al. 2002 355.946 62.16 – -1.58 -2.55 -44.8
Dambis 1999 356.5 62.183 – – – –

💡 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 – – – – – 250* – –
Celli et al. 2024 – – – 10 – 80 – –
Cavallo et al. 2024 2.87 2.04 – 23 0.290 – – –
Hunt & Reffert 2023 3.10 1.96 0.94 12 – – – –
Just et al. 2023 – – – 10 – 107 – –
Cantat-Gaudin & Anders 2020 2.96 – – – – – – –
Cantat-Gaudin et al. 2018 2.96 – – – – – – –
Loktin & Popova 2017 2.14 2.28 – 6 – – – –
Kharchenko et al. 2016 2.40 2.17 – 10 – – – –
Kharchenko et al. 2013 2.40 2.17 – 10 – – – –
Kharchenko et al. 2012 2.40 2.17 – 10 – – – –
van den Bergh 2006 2.14 2.29 – 6 – – – –
Dias et al. 2002 2.14 2.28 – 6 – – – –
Dambis 1999 2.23 2.38 – 5 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2584 27.1 356.44 62.14 0.31 -3.59 -1.56 – 0.27

💡 Note: The % column shows the percentage of members that Stock 17 shares with each listed object.

Visualization
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Stock 17 UCC
Stock 17 HUNT23
Stock 17 CANTAT20
Galactocentric position diagram