Kronberger 85

(SAI 84; MWSC 1395; DSH J0758.3-3446)

Click to load Aladin Lite
0.74 UTI
0.73
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members) 1.2 [arcmin]
  • CN 0.73 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.6 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Kronberger 85 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Extremely distant High extinction Massive Intermediate age

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 119.588 -34.769 0.119 -1.362 2.778 –
Just et al. 2023 119.581 -34.77 – – – –
Cantat-Gaudin et al. 2020 119.59 -34.77 0.069 -1.265 2.815 –
Cantat-Gaudin & Anders 2020 119.59 -34.77 0.069 -1.265 2.815 –
Bica et al. 2019 119.588 -34.764 – – – –
Cantat-Gaudin et al. 2018 119.59 -34.77 0.069 -1.265 2.815 –
Kharchenko et al. 2016 119.581 -34.77 – – – –
Kharchenko et al. 2013 119.586 -34.772 – -0.83 3.66 29.2
Glushkova et al. 2010 119.59 -34.769 – – – –
Kronberger et al. 2006 119.587 -34.77 – – – –
Dias et al. 2002 119.592 -34.769 – -0.83 3.66 –

💡 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
Just et al. 2023 – – – 316 – 2506 – –
Cantat-Gaudin & Anders 2020 10.24 – – – – – – –
Cantat-Gaudin et al. 2018 10.24 – – – – – – –
Kharchenko et al. 2016 10.38 4.52 – 316 – – – –
Kharchenko et al. 2013 10.38 4.52 – 316 – – – –
Glushkova et al. 2010 8.50 3.63 – 631 – – – –
Dias et al. 2002 8.50 3.63 – 631 – – – –

Visualization

â„šī¸