The dense-gas mass versus star formation rate relation: a misleading linearity?
We model the star formation relation of molecular clumps in dependence of their dense-gas mass when their volume density profile is that of an isothermal sphere (i.e., ##IMG## [http://ej.iop.org/images/0004-637X/843/1/7/apjaa7518ieqn1.gif] $\rho _\mathrmclump(r)\propto r^-2$ ). Dense gas is defined...
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| Main Author: | |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
2017 June 26
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| In: |
The astrophysical journal
Year: 2017, Volume: 843, Issue: 1, Pages: 7 |
| ISSN: | 1538-4357 |
| DOI: | 10.3847/1538-4357/aa7518 |
| Online Access: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.3847/1538-4357/aa7518
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| Author Notes: | G. Parmentier |
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The dense-gas mass versus star formation rate relation: a misleading linearity?
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