Collinder 34

Click to load Aladin Lite
0.18 UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.36
Cdup
Stellar density (N50/rad) 26.5 [N/pc2]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.36 Possibly duplicate

Overview

â„šī¸
Collinder 34 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~2.29 kpc) differs significantly from the median photometric distance (~1.39 kpc).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 44.83 60.57 0.437 -0.35 0.041 -55.546
Monteiro & Dias 2019 44.846 60.567 – -0.208 0.122 2.471
Loktin & Popova 2017 44.85 60.567 – 1.433 -0.137 -40.0
Dias et al. 2014 44.846 60.567 – 0.4 0.44 -40.0

💡 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– 1.385 2.085 – 22 0.006 – – –
Monteiro & Dias 2019 1.69 2.01 – 21 0.006 – – –
Loktin & Popova 2017 1.08 2.16 – 24 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
SAI 24 63.8 44.83 60.57 0.45 -0.23 0.07 -49.28 0.91
CWNU 4436 13.8 44.87 60.57 0.23 -0.48 0.1 – 0.04
AFGL 4029 2.1 45.21 60.54 0.44 -0.13 0.03 -30.61 0.14
IRAS 02575+6017 0.5 45.26 60.52 0.42 -0.06 -0.09 -30.61 0.36

💡 Note: The % column shows the percentage of members that Collinder 34 shares with each listed object.

Visualization

â„šī¸