Gaia 8

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0.68 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 30.5 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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Gaia 8 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above 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.

Note: This object shares a large percentage of members with 4 later reported entries. See table with shared members information.

Very 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 – 282.562 33.363 3.447 1.788 -3.886 -18.689
Zhang et al. 2024 282.543 33.393 – – – –
Hunt & Reffert 2024 282.543 33.393 3.436 1.743 -3.955 -21.8
Cavallo et al. 2024 282.474 33.019 3.437 – – –
Hunt & Reffert 2023 282.543 33.393 3.436 1.743 -3.955 -21.8
Bastian 2019 282.52 33.363 – – – –

💡 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 – – – – 0.035* – – –
Hunt & Reffert 2024 – – – – – 73* – –
Cavallo et al. 2024 0.30 0.66 – 14 -0.260 – – –
Hunt & Reffert 2023 0.29 0.18 0.64 21 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
PHOC 41 91.0 282.54 33.38 3.45 1.8 -3.86 -18.69 0.0
OCSN 249 77.4 282.52 33.39 3.46 1.82 -3.87 -18.83 0.0
CWWL 3595 60.9 282.53 33.37 3.47 1.82 -3.87 -18.54 0.0
OCSN 16 3.0 283.65 32.19 2.7 1.17 -3.57 -15.94 0.45

💡 Note: The % column shows the percentage of members that Gaia 8 shares with each listed object.

Visualization

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