XDOCC 07

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0.00 UTI
0.33
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 8.7 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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XDOCC 07 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely 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.

Very close Low extinction Near-solar metallicity Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 159.441 -58.91 2.247 -14.372 0.916 9.484
Jaehnig et al. 2021 159.481 -58.723 2.281 -14.316 0.925 –

💡 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
Piatti et al. 2023 – – – 575 0.240 125 0.43 –
Jaehnig et al. 2021 0.44* 0.58 – 72 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
VDBH 99 100.0 159.52 -59.16 2.23 -14.47 0.99 8.58 1.0
HSC 2356 6.1 159.48 -59.03 2.05 -14.64 1.0 -11.52 0.0

💡 Note: The % column shows the percentage of members that XDOCC 07 shares with each listed object.

Visualization

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