Saloranta 10

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0.62 UTI
0.72
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.4 [arcmin]
  • CN 0.72 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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Saloranta 10 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 81.227 37.576 0.9 0.28 -4.309 14.411
Zhang et al. 2024 81.215 37.566 – – – –
Hunt & Reffert 2024 81.215 37.566 0.896 0.301 -4.312 4.217
Cavallo et al. 2024 81.216 37.547 0.895 – – –
Hunt & Reffert 2023 81.215 37.566 0.896 0.301 -4.312 4.217
Bica et al. 2019 81.22 37.542 – – – –

💡 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
Zhang et al. 2024 – – – – -0.127* – – –
Hunt & Reffert 2024 – – – – – 382* – –
Cavallo et al. 2024 1.10 1.22 – 316 0.110 – – –
Hunt & Reffert 2023 1.05 1.11 0.76 144 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
COIN-Gaia 17 98.9 81.23 37.57 0.89 0.29 -4.31 8.92 0.07
UBC 89 96.8 81.23 37.57 0.9 0.29 -4.3 14.41 0.01

💡 Note: The % column shows the percentage of members that Saloranta 10 shares with each listed object.

Visualization

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