ESO 489 01

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0.18 UTI
0.25
CN
0.04
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.5 [pc], 0.2 [pc-2]
  • CN 0.25 Poorly populated
  • Cdens 0.04 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
ESO 489 01 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a very close* distance, below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~0.31 kpc) differs significantly from the median photometric distance (~2.16 kpc).

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

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.

Dias et al. (2002)
No cluster (Carraro, G. 2016, MNRAS 455, 4031); cat V3.5 (Jan 2016)

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 90.79 -27.207 3.186 -6.544 0.015 3.263
He et al. 2022 90.407 -27.819 3.245 -6.577 -0.154 –
Loktin & Popova 2017 91.245 -26.732 – -0.002 0.08 –
Sampedro et al. 2017 91.242 -26.733 – – – –
Dias et al. 2014 91.242 -26.733 – -0.63 0.33 –

💡 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– 2.16 0.255 – 550 – – – –
He et al. 2022 – 0.15 – 100 – – – –
Loktin & Popova 2017 2.16 0.36 – 1000 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 229 80.0 90.59 -27.98 3.2 -6.52 -0.17 2.03 0.11
OCSN 81 72.0 91.01 -27.1 3.19 -6.59 0.26 3.26 0.01

💡 Note: The % column shows the percentage of members that ESO 489 01 shares with each listed object.

Visualization

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