[CII] as a star formation rate tracer in M31: Is [CII]/TIR the best photoelectric heating efficiency proxy?
February 01, 2018
The [CII] 158$\mu$m line is typically the brightest far-IR emission line from star-forming galaxies. To use this line as a tracer of star-formation and a diagnostic of the ISM conditions, we must understand details of the heating mechanisms generating it and contributing to the total observed emission, especially the photoelectric (PE) heating mechanism.
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating
very compact bibliographies which can be beneficial to authors and
readers, and in "proceeding" format
which is more detailed and complete.