Saurer 1

(FSR 1184; MWSC 1184)

Click to load Aladin Lite
0.39 UTI
0.0
CN
0.16
Cdens
0.38
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members) 1.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.38 Low quality
  • Clit 0.7 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Saurer 1 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very large distance, well above the mid-plane, affected by low extinction. It is catalogued as an extremely massive, near-solar metallicity, old cluster (see Parameters). It is moderately studied in the literature.
Extremely distant Low extinction Extremely massive Near-solar metallicity Old

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 110.229 1.811 0.083 -0.305 -0.352 103.402
He et al. 2023 110.232 1.813 0.072 -0.263 -0.332 103.4
Just et al. 2023 110.226 1.802 – – – –
Perren et al. 2022 110.225 1.8 – – – –
Donor et al. 2020 110.234 1.8 – -0.36 -0.39 105.0
Bica et al. 2019 110.237 1.809 – – – –
Kharchenko et al. 2016 110.226 1.802 – – – –
Kharchenko et al. 2013 110.233 1.8 – 3.46 -6.73 95.3
Gozha et al. 2012 110.233 1.808 – – – –
Kharchenko et al. 2007 110.23 1.81 – 0.02 – –
Froebrich et al. 2007 105.679 -11.461 – – – –
van den Bergh 2006 110.225 1.8 – – – –
Dias et al. 2002 110.233 1.808 – 3.46 -6.73 98.0

💡 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] Bfr BSS
He et al. 2023 15.85 0.65 – 2512 – – – –
Just et al. 2023 – – – 3981 – 10162 – –
Perren et al. 2022 12.36 0.40 – 6607 -0.080 10000 0.81 –
Donor et al. 2020 – – – – -0.420 – – –
Kharchenko et al. 2016 13.72 0.13 – 3981 – – – –
Kharchenko et al. 2013 13.72 0.13 – 3981 -0.380 – – –
Gozha et al. 2012 13.20 – – 5012 -0.380 – – –
van den Bergh 2006 11.97 0.37 – 7079 – – – –
Dias et al. 2002 13.20 0.43 – 5012 -0.380 – – –

Visualization

â„šī¸