HSC 291

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0.40 UTI
0.26
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 291 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

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

Distant High extinction Metal-rich Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 282.535 -4.103 0.281 0.546 -1.659 44.645
Hunt & Reffert 2024 282.535 -4.1 0.289 0.538 -1.652 45.7
Cavallo et al. 2024 282.534 -4.103 0.287 – – –
Hunt & Reffert 2023 282.535 -4.1 0.289 0.538 -1.652 45.7

💡 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 – – – – – 647* – –
Cavallo et al. 2024 3.31 4.59 – 78 0.950 – – –
Hunt & Reffert 2023 3.00 5.13 2.13 111 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3100 100.0 282.53 -4.12 0.3 0.52 -1.66 39.92 0.21

💡 Note: The % column shows the percentage of members that HSC 291 shares with each listed object.

Visualization

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