UBC 1618

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0.00 UTI
0.4
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 6.3 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
UBC 1618 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Very young

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 – 125.775 -37.58 0.808 -5.692 5.278 27.375
Hunt & Reffert 2024 125.774 -37.583 0.809 -5.742 5.293 30.496
Cavallo et al. 2024 125.79 -37.606 0.809 – – –
Hunt & Reffert 2023 125.774 -37.583 0.809 -5.742 5.293 30.496
Castro-Ginard et al. 2022 125.8 -37.59 0.8 -5.71 5.27 –

💡 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
Hunt & Reffert 2024 – – – – – 114* – –
Cavallo et al. 2024 1.26 0.89 – 13 0.270 – – –
Hunt & Reffert 2023 1.20 0.48 1.57 11 – – – –
Castro-Ginard et al. 2022 1.32 0.30 – 33 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Casado 4 100.0 125.77 -37.58 0.81 -5.7 5.28 28.09 0.46

💡 Note: The % column shows the percentage of members that UBC 1618 shares with each listed object.

Visualization

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