We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.
To save content items to your account,
please confirm that you agree to abide by our usage policies.
If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account.
Find out more about saving content to .
To save content items to your Kindle, first ensure [email protected]
is added to your Approved Personal Document E-mail List under your Personal Document Settings
on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part
of your Kindle email address below.
Find out more about saving to your Kindle.
Note you can select to save to either the @free.kindle.com or @kindle.com variations.
‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi.
‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
The stellar Initial Mass Function (IMF) can be conveniently represented as a canonical two-part power law function and is largely invariant for star formation regions evident in the Local Group of galaxies. The lack of massive stars in regions of low star formation density and other evidence imply that the IMF is not a probability density distribution function, but is instead closer to an optimal density distribution function. Binary stars and stellar dynamics have a very significant influence on the counts of low-mass stars and need to be corrected for. This chapter offers a review of how recent advancements in the measurement of the IMF from detailed star counts in different environments (e.g., young massive clusters, globular clusters, elliptical galaxies and ultrafaint dwarf galaxies), properly interpreted via detailed numerical models, indicate that the environmental conditions and metallicity both have an impact on the shape of the IMF.
Recommend this
Email your librarian or administrator to recommend adding this to your organisation's collection.