Stellar collisions in globular clusters: Constraints on the initial mass function of the first generation of stars

Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/202243556e]

Fig. 3.

Shape of the IMF for various values of the intermediate slope, α₁, around the Galactic field value of −1.3. The values of α₀ and α₂ are set to the Galactic field values of −0.3 and −2.3, respectively. The mass functions are normalized assuming the same arbitrary mass.

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