HSC 2907

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0.41 UTI
0.85
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.73
Cdup
Radius (P>50% members) 70.2 [arcmin]
  • CN 0.85 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.73 Likely unique

Overview

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HSC 2907 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

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

Very close Moderate extinction Near-solar metallicity Very 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 – 244.86 -24.989 6.365 -10.631 -21.498 -5.444
Hunt & Reffert 2024 244.773 -24.45 6.361 -10.679 -21.702 -6.463
Cavallo et al. 2024 244.859 -25.146 6.365 – – –
Hunt & Reffert 2023 244.773 -24.45 6.361 -10.679 -21.702 -6.463

💡 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 – – – – – 133* – –
Cavallo et al. 2024 0.16 2.22 – 7 -0.230 – – –
Hunt & Reffert 2023 0.15 0.55 1.08 10 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14698 27.3 244.65 -25.04 6.28 -10.79 -21.61 -4.49 0.43
OCSN 246 16.9 245.41 -24.73 6.71 -10.64 -22.4 -3.67 0.45
OCSN 96 0.8 240.86 -22.58 7.02 -11.74 -23.9 -7.43 0.67

💡 Note: The % column shows the percentage of members that HSC 2907 shares with each listed object.

Visualization

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