HSC 1995

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0.00 UTI
0.25
CN
1.0
Cdens
0.5
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
HSC 1995 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported 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.

Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 121.761 -29.895 0.6 -3.619 3.603 33.389
Hunt & Reffert 2024 121.761 -29.887 0.597 -3.639 3.619 47.231
Cavallo et al. 2024 121.765 -29.913 0.597 – – –
Hunt & Reffert 2023 121.761 -29.887 0.597 -3.639 3.619 47.231

💡 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
Hunt & Reffert 2024 – – – – – 194* – –
Cavallo et al. 2024 1.49 0.63 – 186 -0.230 – – –
Hunt & Reffert 2023 1.60 0.23 0.63 521 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
XDOCC 05 100.0 121.76 -29.89 0.6 -3.62 3.6 35.87 0.45
OC 0433 96.0 121.79 -29.89 0.6 -3.61 3.61 33.39 0.0

💡 Note: The % column shows the percentage of members that HSC 1995 shares with each listed object.

Visualization

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