HSC 2950

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0.51 UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.1 [arcmin]
  • CN 0.78 Rich
  • 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 2950 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by very high extinction. It is catalogued as a very massive, metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~3.43 kpc) differs significantly from the median photometric distance (~2.50 kpc).

Note: This object shares a very small percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Very high extinction Very massive Metal-poor Intermediate age

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 264.268 -32.495 0.292 -0.514 -2.195 -19.959
Hunt & Reffert 2024 264.27 -32.496 0.304 -0.51 -2.209 -3.31
Cavallo et al. 2024 264.269 -32.483 0.304 – – –
Hunt & Reffert 2023 264.27 -32.496 0.304 -0.51 -2.209 -3.31

💡 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 – – – – – 6111* – –
Cavallo et al. 2024 2.09 5.33 – 145 -0.760 – – –
Hunt & Reffert 2023 2.92 5.34 3.13 129 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Trumpler 28a 7.5 264.29 -32.48 0.28 -0.33 -1.87 – 0.03
Trumpler 28b 5.3 264.25 -32.47 0.26 -0.93 -2.52 -12.36 0.29

💡 Note: The % column shows the percentage of members that HSC 2950 shares with each listed object.

Visualization

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