VVV 095

(VVV-CL 095)

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0.11 UTI
0.0
CN
0.03
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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VVV 095 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

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.

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 257.766 -39.669 0.275 -2.137 -3.354 -13.061
Bica et al. 2019 257.726 -39.692 – – – –
Morales et al. 2013 257.729 -39.697 – – – –
Borissova et al. 2011 257.729 -39.697 – – – –

💡 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– 3.0 – – 200 – – – –
Morales et al. 2013 3.00 – – 200 – – – –

Visualization

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