Stock 16

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0.48 UTI
0.31
CN
0.1
Cdens
0.25
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.31 Poorly populated
  • Cdens 0.1 Very loose
  • CC3 0.25 Low quality
  • Clit 0.87 Well-studied
  • Cdup 1.0 Unique

Overview

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Stock 16 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is well-studied in the literature.

(*): The parallax distance estimate (~4.40 kpc) differs significantly from the median photometric distance (~1.81 kpc).

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 199.773 -62.615 0.228 -6.54 -0.972 -31.499
Celli et al. 2024 199.86 -62.622 – – – –
Jaehnig et al. 2021 199.682 -62.583 0.501 -4.178 -1.796 –
Rain et al. 2021 199.86 -62.622 0.222 -6.574 -0.991 –
Cantat-Gaudin et al. 2020 199.86 -62.622 0.222 -6.574 -0.991 –
Cantat-Gaudin & Anders 2020 199.86 -62.622 0.222 -6.574 -0.991 –
Soubiran et al. 2018 199.86 -62.622 – – – -38.11
Cantat-Gaudin et al. 2018 199.86 -62.622 0.222 -6.574 -0.991 –
Loktin & Popova 2017 199.875 -62.633 – -8.407 2.036 -41.8
Dias et al. 2014 199.871 -62.633 – -8.97 -3.36 –
Morales et al. 2013 199.871 -62.633 – – – –
Gozha et al. 2012 199.871 -62.633 – – – –
Piskunov et al. 2008 199.691 -62.505 – – – –
Kharchenko et al. 2007 199.87 -62.63 – 0.22 – -41.8
van den Bergh 2006 199.7 -62.517 – – – –
Kharchenko et al. 2005 199.69 -62.51 – -3.31 -0.03 -41.8
Kharchenko et al. 2003 199.69 -62.51 – -3.58 0.15 –
Dias et al. 2002 199.871 -62.633 – -8.97 -3.36 -41.8
Dambis 1999 199.871 -62.633 – – – –

💡 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] Bfrac BSS
UCC 99999– 1.81 1.505 – 8 – 876 – 0.0
Celli et al. 2024 – – – 6 – 340 – –
Jaehnig et al. 2021 1.99(1) – – – – – – –
Rain et al. 2021 3.99 1.61 – 8 – – – 0
Cantat-Gaudin & Anders 2020 3.99 – – – – – – –
Soubiran et al. 2018 3.99 – – – – – – –
Cantat-Gaudin et al. 2018 3.99 – – – – – – –
Loktin & Popova 2017 1.66 1.54 – 8 – – – –
Morales et al. 2013 1.81 – – 8 – – – –
Gozha et al. 2012 1.81 – – 8 – 1413 – –
Piskunov et al. 2008 1.64 1.49 – 6 – – – –
van den Bergh 2006 1.64 1.52 – 8 – – – –
Kharchenko et al. 2005 1.64 1.49 – 6 – – – –
Kharchenko et al. 2003 1.64 1.24 – – – – – –
Dias et al. 2002 1.81 1.61 – 8 – – – –
Dambis 1999 1.85 1.45 – 3 – – – –

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

Visualization

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