Carraro 1

(MWSC 1829)

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0.33 UTI
0.36
CN
0.02
Cdens
0.25
CC3
0.5
Clit
1.0
Cdup
Core radius and density 4.2 [pc], 0.1 [pc-2]
  • CN 0.36 Poorly populated
  • Cdens 0.02 Very loose
  • CC3 0.25 Low quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Carraro 1 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.12 kpc) differs significantly from the median photometric distance (~1.79 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 159.274 -58.732 0.32 -5.984 2.399 –
Just et al. 2023 159.226 -58.746 – – – –
Bica et al. 2019 159.238 -58.753 – – – –
Dias et al. 2018 – – – -8.43 2.48 –
Sampedro et al. 2017 159.25 -58.733 – -5.24 -1.92 –
Joshi et al. 2016 159.232 -58.75 – – – –
Kharchenko et al. 2016 159.226 -58.746 – – – –
Dias et al. 2014 159.25 -58.733 – -6.74 -2.51 –
Kharchenko et al. 2013 159.232 -58.75 – -7.11 -2.01 -8.5
van den Bergh 2006 159.25 -58.733 – – – –
Dias et al. 2002 159.25 -58.733 – -6.74 -2.51 -8.5

💡 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– 1.79 0.85 – 1259 – 16 – –
Just et al. 2023 – – – 1259 – 16 – –
Joshi et al. 2016 1.79 0.85 – 1259 – – – –
Kharchenko et al. 2016 1.79 0.85 – 1259 – – – –
Kharchenko et al. 2013 1.79 0.85 – 1259 – – – –
van den Bergh 2006 1.90 0.79 – 3020 – – – –
Dias et al. 2002 1.90 0.79 – 3020 – – – –

Visualization

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