Collinder 316

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0.28 UTI
0.62
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.53
Cdup
Stellar density (N50/rad) 23.0 [N/pc2]
  • CN 0.62 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.53 Likely unique

Overview

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Collinder 316 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close* distance, above the mid-plane, affected by low extinction. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 12 years.

(*): The parallax distance estimate (~1.65 kpc) differs significantly from the median photometric distance (~1.00 kpc).

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 253.697 -40.76 0.604 -0.284 -1.289 -24.59
Dias et al. 2014 253.875 -40.833 – -2.26 -3.39 -29.05
Kharchenko et al. 2003 253.68 -40.76 – -0.89 -4.33 –

💡 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– 1.0 0.62 – – – – – –
Kharchenko et al. 2003 1.00 0.62 – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 323 78.1 253.97 -40.69 0.59 -0.23 -1.25 -21.03 0.37
ESO 332 08 46.6 253.7 -40.76 0.58 -0.27 -1.34 -18.45 0.65
OC 0674 34.2 253.7 -40.77 0.6 -0.28 -1.29 -22.14 0.0

💡 Note: The % column shows the percentage of members that Collinder 316 shares with each listed object.

Visualization

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