HSC 640

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0.48 UTI
0.81
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.78
Cdup
Radius (P>50% members) 7.4 [arcmin]
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.78 Very likely unique

Overview

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HSC 640 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Massive Near-solar metallicity Very young

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 309.736 42.147 0.678 -2.319 -3.43 1.133
Zhang et al. 2024 309.774 42.12 – – – –
Hunt & Reffert 2024 309.774 42.12 0.654 -2.356 -3.44 11.588
Cavallo et al. 2024 309.557 42.408 0.65 – – –
Hunt & Reffert 2023 309.774 42.12 0.654 -2.356 -3.44 11.588

💡 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 – – – – -0.102* – – –
Hunt & Reffert 2024 – – – – – 1795* – –
Cavallo et al. 2024 1.70 4.43 – 16 0.620 – – –
Hunt & Reffert 2023 1.49 5.05 3.09 14 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
DB2001 16 21.8 309.65 42.11 0.69 -2.53 -3.27 114.81 0.44
FSR 0245 9.6 309.69 42.15 0.69 -1.91 -3.61 21.62 0.52
OC 0131 6.9 309.63 42.48 0.63 -2.37 -3.34 -11.77 0.12
FSR 0249 5.0 309.63 42.49 0.62 -2.37 -3.31 -23.49 0.63

💡 Note: The % column shows the percentage of members that HSC 640 shares with each listed object.

Visualization

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