Shorlin 1

(MWSC 1891)

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0.59 UTI
0.33
CN
1.0
Cdens
0.75
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members) 0.4 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.44 Poorly studied
  • Cdup 1.0 Unique

Overview

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Shorlin 1 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Very distant Moderate extinction Very young

Dias et al. (2002)
Asterism (Turner, D. G. 2012, Ap&SS 337, 303)

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 166.447 -61.228 0.108 -5.902 2.199 151.959
Celli et al. 2024 166.443 -61.231 – – – –
Just et al. 2023 166.572 -61.239 – – – –
Cantat-Gaudin et al. 2020 166.443 -61.231 0.083 -5.869 2.189 –
Cantat-Gaudin & Anders 2020 166.443 -61.231 0.083 -5.869 2.189 –
Cantat-Gaudin et al. 2018 166.443 -61.231 0.083 -5.869 2.189 –
Kharchenko et al. 2016 166.572 -61.239 – – – –
Kharchenko et al. 2013 166.579 -61.243 – -5.4 -0.16 –

💡 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
Celli et al. 2024 – – – 3 – 211 – –
Just et al. 2023 – – – 3 – 1365 – –
Cantat-Gaudin & Anders 2020 8.89 – – – – – – –
Cantat-Gaudin et al. 2018 8.89 – – – – – – –
Kharchenko et al. 2016 5.59 2.52 – 3 – – – –
Kharchenko et al. 2013 5.59 2.52 – 3 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0559 45.5 166.45 -61.23 0.11 -5.9 2.2 93.75 0.08

💡 Note: The % column shows the percentage of members that Shorlin 1 shares with each listed object.

Visualization

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