Constraining the thin disc initial mass function using galactic classical Cepheids
<i>Context. <i/>The initial mass function (IMF) plays a crucial role in galaxy evolution and its implications on star formation theory make it a milestone for the next decade. It is in the intermediate and high mass ranges where the uncertainties of the IMF are larger. This is a major su...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
21 February 2017
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| In: |
Astronomy and astrophysics
Year: 2017, Volume: 599 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201629464 |
| Online Access: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201629464
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| Author Notes: | R. Mor, A.C. Robin, F. Figueras, and B. Lemasle |
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Constraining the thin disc initial mass function using galactic classical Cepheids
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