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.
Name | Age (Myr) | Mecl (M⊙) | rh (pc) | ρecl (M⊙ pc−3) | α3 | References |
Arches | 2–3 | 1.3 × 104 | 0.24 | 1.12 × 105 | 1.65–2.3 | 1–6 |
NGC 3606 | 1–3 | 0.7 × 104 | 0.2 | 1.04 × 105 | 1.9–2.3 | 3, 4, 7–9 |
Wd1 | 3–4 | 5 × 104 | 1 | 5.96 × 103 | 1.6–2.3 | 10 |
R136 | 2–3 | 105 | 1.1 | 8.97 × 103 | 2.2–2.6 | 11–13 |
Name | Age (Myr) | Mecl (M⊙) | rh (pc) | ρecl (M⊙ pc−3) | α3 | References |
Arches | 2–3 | 1.3 × 104 | 0.24 | 1.12 × 105 | 1.65–2.3 | 1–6 |
NGC 3606 | 1–3 | 0.7 × 104 | 0.2 | 1.04 × 105 | 1.9–2.3 | 3, 4, 7–9 |
Wd1 | 3–4 | 5 × 104 | 1 | 5.96 × 103 | 1.6–2.3 | 10 |
R136 | 2–3 | 105 | 1.1 | 8.97 × 103 | 2.2–2.6 | 11–13 |
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).
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.
Name | Age (Myr) | Mecl (M⊙) | rh (pc) | ρecl (M⊙ pc−3) | α3 | References |
Arches | 2–3 | 1.3 × 104 | 0.24 | 1.12 × 105 | 1.65–2.3 | 1–6 |
NGC 3606 | 1–3 | 0.7 × 104 | 0.2 | 1.04 × 105 | 1.9–2.3 | 3, 4, 7–9 |
Wd1 | 3–4 | 5 × 104 | 1 | 5.96 × 103 | 1.6–2.3 | 10 |
R136 | 2–3 | 105 | 1.1 | 8.97 × 103 | 2.2–2.6 | 11–13 |
Name | Age (Myr) | Mecl (M⊙) | rh (pc) | ρecl (M⊙ pc−3) | α3 | References |
Arches | 2–3 | 1.3 × 104 | 0.24 | 1.12 × 105 | 1.65–2.3 | 1–6 |
NGC 3606 | 1–3 | 0.7 × 104 | 0.2 | 1.04 × 105 | 1.9–2.3 | 3, 4, 7–9 |
Wd1 | 3–4 | 5 × 104 | 1 | 5.96 × 103 | 1.6–2.3 | 10 |
R136 | 2–3 | 105 | 1.1 | 8.97 × 103 | 2.2–2.6 | 11–13 |
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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