UBC 257

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0.02 UTI
0.74
CN
0.16
Cdens
0.75
CC3
0.0
Clit
0.05
Cdup
Core radius and density 4.9 [pc], 0.8 [pc-2]
  • CN 0.74 Moderately populated
  • Cdens 0.16 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.05 Very likely duplicate

Overview

â„šī¸
UBC 257 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 6 years.

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.

Castro-Ginard et al. (2020)
Coincidence with Sim et al. (2019, J. Korean Astron. Soc., 52, 145) or Liu & Pang (2019ApJS..245...32L), see Sect. 4.1.5.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 153.194 -60.898 0.488 -6.349 3.082 -11.901
Castro-Ginard et al. 2020 153.185 -60.893 0.47 -6.32 3.073 –

💡 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– 1.89 0.85 – 85 – – – –
Kounkel et al. 2020 1.89 0.85 – 85 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2059 94.9 153.21 -60.91 0.49 -6.36 3.08 -11.96 0.41
CWWDL 13311 83.7 153.17 -60.9 0.49 -6.36 3.11 -11.97 0.06
OC 0540 57.1 153.19 -60.93 0.5 -6.34 3.09 -11.9 0.01

💡 Note: The % column shows the percentage of members that UBC 257 shares with each listed object.

Visualization

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