Collinder 228

Click to load Aladin Lite
0.79 UTI
0.62
CN
1.0
Cdens
0.75
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad) 11.5 [N/pc2]
  • CN 0.62 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.78 Well-studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Collinder 228 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.

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

Cavallo et al. (2024)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 161.009 -60.09 0.399 -6.698 1.921 -11.487
Hunt & Reffert 2024 161.011 -60.091 0.399 -6.668 1.92 -28.406
Cavallo et al. 2024 161.013 -60.081 0.399 – – –
Hunt & Reffert 2023 161.011 -60.091 0.399 -6.668 1.92 -28.406
Loktin & Popova 2017 160.995 -60.087 – -6.55 2.03 -13.5
Dias et al. 2014 161.0 -60.087 – -6.31 0.12 –
Gozha et al. 2012 161.0 -60.087 – – – –
Piskunov et al. 2008 160.939 -60.085 – – – –
Kharchenko et al. 2007 160.99 -60.09 – 0.35 – -13.46
van den Bergh 2006 160.95 -60.083 – – – –
Kharchenko et al. 2005 160.95 -60.09 – -6.66 1.93 -13.46
Kharchenko et al. 2003 160.99 -60.09 – -6.3 2.67 –
Chen et al. 2003 160.749 -59.966 – -6.55 2.03 -12.0
Dias et al. 2002 161.0 -60.087 – -6.55 2.03 -10.71
Dambis 1999 161.0 -60.087 – – – –

💡 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– 2.2 0.96 1.06 6 -0.140 2975 – –
Hunt & Reffert 2024 – – – – – 327(1) – –
Cavallo et al. 2024 1.91 0.58 – 59 -0.140 – – –
Hunt & Reffert 2023 2.32 0.96 1.06 5 – – – –
Loktin & Popova 2017 1.91 1.05 – 7 – – – –
Gozha et al. 2012 2.20 – – 7 – 5623 – –
Piskunov et al. 2008 1.91 0.81 – 5 – – – –
van den Bergh 2006 2.20 1.05 – 7 – – – –
Kharchenko et al. 2005 1.91 0.81 – 5 – – – –
Kharchenko et al. 2003 2.22 0.93 – – – – – –
Chen et al. 2003 2.20 – – 0 – – – –
Dias et al. 2002 2.20 1.06 – 7 – – – –
Dambis 1999 2.29 1.04 – 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
OC 0550 33.3 161.01 -60.1 0.4 -6.61 1.9 -28.44 0.0

💡 Note: The % column shows the percentage of members that Collinder 228 shares with each listed object.

Visualization

â„šī¸