FSR 0291

(MWSC 3489)

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0.59 UTI
0.47
CN
1.0
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 1.1 [arcmin]
  • CN 0.47 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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FSR 0291 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~7.67 kpc) differs significantly from the median photometric distance (~5.14 kpc).

Very distant High extinction Near-solar metallicity Intermediate age

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 – 319.084 48.348 0.13 -3.178 -4.204 –
Hunt & Reffert 2024 319.079 48.354 0.145 -3.171 -4.193 –
Cavallo et al. 2024 319.091 48.351 0.139 – – –
He et al. 2023 319.082 48.349 0.136 -3.215 -4.242 –
Hunt & Reffert 2023 319.079 48.354 0.145 -3.171 -4.193 –
Bica et al. 2019 319.089 48.36 – – – –
Froebrich et al. 2007 319.083 48.362 – – – –

💡 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 – – – – – 963* – –
Cavallo et al. 2024 5.94 4.44 – 295 0.300 – – –
He et al. 2023 4.68 4.70 – 1585 – – – –
Hunt & Reffert 2023 5.14 4.78 2.19 110 – – – –

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

Visualization

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