Saurer 3

(MWSC 1839)

Click to load Aladin Lite
0.76 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members) 1.6 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.65 Moderately studied
  • Cdup 1.0 Unique

Overview

ℹ️
Saurer 3 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very massive, near-solar metallicity, old cluster (see Parameters). It is moderately studied in the literature.
Very distant Moderate extinction Very massive Near-solar metallicity Old

Cavallo et al. (2024)
Gold sample.

Data

ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 160.354 -55.29 0.142 -6.682 3.263 39.802
Hu & Soubiran 2025 160.394 -55.303 – – – –
Hunt & Reffert 2024 160.348 -55.288 0.108 -6.681 3.262 –
Cavallo et al. 2024 160.394 -55.303 0.13 – – –
He et al. 2023 160.351 -55.29 0.135 -6.668 3.259 –
Hunt & Reffert 2023 160.348 -55.288 0.108 -6.681 3.262 –
Perren et al. 2022 160.375 -55.3 – – – –
SΓ‘nchez et al. 2020 160.354 -55.306 – -6.836 3.34 –
Bica et al. 2019 160.339 -55.288 – – – –
Dias et al. 2014 160.354 -55.306 – -6.73 -1.62 –
van den Bergh 2006 160.375 -55.3 – – – –
Dias et al. 2002 160.354 -55.306 – -6.73 -1.62 –

πŸ’‘ 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
Hu & Soubiran 2025 – – – – -0.330* – – –
Hunt & Reffert 2024 – – – – – 626* – –
Cavallo et al. 2024 10.23 1.91 – 2138 -0.100 – – –
He et al. 2023 6.76 2.30 – 2512 – – – –
Hunt & Reffert 2023 5.65 2.47 1.56 1033 – – – –
Perren et al. 2022 6.14 2.20 – 6457 0.020 14000 0.86 –
van den Bergh 2006 8.83 1.92 – 2818 – – – –
Dias et al. 2002 9.55 2.36 – 1995 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

ℹ️