FSR 1527

(MWSC 1765)

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0.68 UTI
0.61
CN
0.96
Cdens
0.75
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 5.3 [arcmin]
  • CN 0.61 Moderately populated
  • Cdens 0.96 Very dense
  • CC3 0.75 High quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

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FSR 1527 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
Relatively close High extinction Near-solar metallicity Very young

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 – 151.654 -57.421 0.398 -7.98 4.436 -17.952
Hunt & Reffert 2024 151.653 -57.427 0.395 -7.962 4.402 -10.594
Cavallo et al. 2024 151.702 -57.444 0.399 – – –
He et al. 2023 151.667 -57.422 0.393 -7.975 4.443 20.19
Hunt & Reffert 2023 151.653 -57.427 0.395 -7.962 4.402 -10.594
Just et al. 2023 151.628 -57.41 – – – –
Bica et al. 2019 151.637 -57.417 – – – –
Kharchenko et al. 2016 151.628 -57.41 – – – –
Kharchenko et al. 2013 151.633 -57.414 – -3.42 5.27 –
Froebrich et al. 2007 151.633 -57.414 – – – –

💡 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 – – – – – 595* – –
Cavallo et al. 2024 2.28 2.17 – 71 0.290 – – –
He et al. 2023 2.88 3.40 – 3 – – – –
Hunt & Reffert 2023 2.42 2.48 2.73 14 – – – –
Just et al. 2023 – – – 2 – 121 – –
Kharchenko et al. 2016 3.26 3.23 – 2 – – – –
Kharchenko et al. 2013 3.26 3.23 – 2 – – – –

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

Visualization

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