Ruprecht 49

(MWSC 1423; OCL 676; ESO 494 15)

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0.67 UTI
0.53
CN
1.0
Cdens
0.5
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.53 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.65 Moderately studied
  • Cdup 1.0 Unique

Overview

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Ruprecht 49 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~2.72 kpc) differs significantly from the median photometric distance (~1.82 kpc).

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

Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 120.819 -26.767 0.368 -3.509 3.841 28.95
Hunt & Reffert 2024 120.812 -26.766 0.369 -3.487 3.835 23.994
Cavallo et al. 2024 120.819 -26.796 0.373 – – –
Hunt & Reffert 2023 120.812 -26.766 0.369 -3.487 3.835 23.994
Just et al. 2023 120.799 -26.767 – – – –
Bica et al. 2019 120.807 -26.775 – – – –
Loktin & Popova 2017 120.81 -26.767 – -4.74 1.01 –
Kharchenko et al. 2016 120.799 -26.767 – – – –
Dias et al. 2014 120.812 -26.767 – -0.95 2.45 –
Kharchenko et al. 2013 120.805 -26.77 – -4.96 0.96 –
van den Bergh 2006 120.812 -26.773 – – – –
Dias et al. 2002 120.812 -26.767 – -4.74 1.01 –

💡 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 – – – – – 298* – –
Cavallo et al. 2024 2.70 1.32 – 162 -0.080 – – –
Hunt & Reffert 2023 2.36 0.63 2.05 474 – – – –
Just et al. 2023 – – – 166 – 43 – –
Loktin & Popova 2017 1.82 0.80 – 85 – – – –
Kharchenko et al. 2016 1.75 0.84 – 166 – – – –
Kharchenko et al. 2013 1.75 0.84 – 166 – – – –
van den Bergh 2006 1.82 0.81 – 85 – – – –
Dias et al. 2002 1.82 0.80 – 85 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1398 69.6 120.82 -26.77 0.37 -3.51 3.85 28.95 0.0

💡 Note: The % column shows the percentage of members that Ruprecht 49 shares with each listed object.

Visualization

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