HSC 1242

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0.40 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1242 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, 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.

Very distant High extinction Massive Near-solar metallicity Young

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 – 68.81 47.288 0.172 0.487 -0.854 –
Hunt & Reffert 2024 68.784 47.277 0.138 0.487 -0.835 –
Cavallo et al. 2024 68.796 47.303 0.135 – – –
Hunt & Reffert 2023 68.784 47.277 0.138 0.487 -0.835 –

💡 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 – – – – – 1861* – –
Cavallo et al. 2024 4.49 3.77 – 105 0.310 – – –
Hunt & Reffert 2023 7.25 4.26 1.53 53 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3059 100.0 68.82 47.29 0.17 0.48 -0.85 -44.76 0.38

💡 Note: The % column shows the percentage of members that HSC 1242 shares with each listed object.

Visualization

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