UBC 1557

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0.54 UTI
0.46
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.46 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1557 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity 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 – 251.042 -45.53 0.388 -1.37 -2.53 -31.39
Hunt & Reffert 2024 251.05 -45.525 0.391 -1.358 -2.545 -12.95
Cavallo et al. 2024 251.032 -45.538 0.391 – – –
Hunt & Reffert 2023 251.05 -45.525 0.391 -1.358 -2.545 -12.95
Castro-Ginard et al. 2022 251.04 -45.53 0.39 -1.37 -2.54 –

💡 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 – – – – – 919* – –
Cavallo et al. 2024 1.73 3.29 – 59 -0.340 – – –
Hunt & Reffert 2023 2.31 2.90 1.44 69 – – – –
Castro-Ginard et al. 2022 2.59 2.62 – 28 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 1600 97.8 251.04 -45.53 0.39 -1.37 -2.53 -31.39 0.1

💡 Note: The % column shows the percentage of members that UBC 1557 shares with each listed object.

Visualization

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