Table 2

Properties of starburst clusters in the MW and the LMC. From left to right the columns denote the cluster name, its age, stellar mass, Mecl, half-mass radius, rh, stellar density, ρecl, within rh, and range of published high-mass PDMF slopes, α3, from the references given in the last column.

NameAge (Myr)Mecl (M)rh (pc)ρecl (M pc−3)α3References
Arches2–31.3 × 1040.241.12 × 1051.65–2.31–6
NGC 36061–30.7 × 1040.21.04 × 1051.9–2.33, 4, 7–9
Wd13–45 × 10415.96 × 1031.6–2.310
R1362–31051.18.97 × 1032.2–2.611–13
NameAge (Myr)Mecl (M)rh (pc)ρecl (M pc−3)α3References
Arches2–31.3 × 1040.241.12 × 1051.65–2.31–6
NGC 36061–30.7 × 1040.21.04 × 1051.9–2.33, 4, 7–9
Wd13–45 × 10415.96 × 1031.6–2.310
R1362–31051.18.97 × 1032.2–2.611–13

1Figer et al. (1999), 2Stolte et al. (2002), 3Stolte et al. (2005), 4Stolte et al. (2006), 5Kim et al. (2006),

6Espinoza et al. (2009), 7Nürnberger & Petr-Gotzens (2002), 8Sung & Bessell (2004), 9Harayama et al. (2008),

10Brandner et al. (2008), 11Andersen et al. (2009), 12Brandl et al. (1996) and 13Massey & Hunter (1998).

Table 2

Properties of starburst clusters in the MW and the LMC. From left to right the columns denote the cluster name, its age, stellar mass, Mecl, half-mass radius, rh, stellar density, ρecl, within rh, and range of published high-mass PDMF slopes, α3, from the references given in the last column.

NameAge (Myr)Mecl (M)rh (pc)ρecl (M pc−3)α3References
Arches2–31.3 × 1040.241.12 × 1051.65–2.31–6
NGC 36061–30.7 × 1040.21.04 × 1051.9–2.33, 4, 7–9
Wd13–45 × 10415.96 × 1031.6–2.310
R1362–31051.18.97 × 1032.2–2.611–13
NameAge (Myr)Mecl (M)rh (pc)ρecl (M pc−3)α3References
Arches2–31.3 × 1040.241.12 × 1051.65–2.31–6
NGC 36061–30.7 × 1040.21.04 × 1051.9–2.33, 4, 7–9
Wd13–45 × 10415.96 × 1031.6–2.310
R1362–31051.18.97 × 1032.2–2.611–13

1Figer et al. (1999), 2Stolte et al. (2002), 3Stolte et al. (2005), 4Stolte et al. (2006), 5Kim et al. (2006),

6Espinoza et al. (2009), 7Nürnberger & Petr-Gotzens (2002), 8Sung & Bessell (2004), 9Harayama et al. (2008),

10Brandner et al. (2008), 11Andersen et al. (2009), 12Brandl et al. (1996) and 13Massey & Hunter (1998).

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