We present a new analysis of the minimum mass for star formation, based on opacity-limited fragmentation. Our analysis differs from the standard one, which considers hierarchical fragmentation of a three-dimensional medium, and yield
The gravitational collapse of a primordial cloud does differ of the gravitational collapse of normal...
In turbulent fragmentation, star formation occurs in condensations created by converging flows. The ...
In turbulent fragmentation, star formation occurs in condensations created by converging flows. The ...
We present a new analysis of the minimum mass for star formation, based on opacity-limited fragmenta...
We present a new analysis of the minimum mass for star formation, based on opacity-limited fragmenta...
We present a new analysis of the minimum mass for star formation, based on opacity-limited fragment...
We present a new analysis of the minimum mass for star formation, based on opacity-limited fragment...
We present a new analysis of the minimum mass for star formation, based on opacity-limited fragmenta...
Context.The minimum mass for star formation is a critical parameter with profound astrophysical, cos...
Context.The minimum mass for star formation is a critical parameter with profound astrophysical, cos...
Theory and simulations suggest that it is possible to form low mass stars via disc fragmentation.The...
As star-forming clouds collapse, the gas within them fragments to ever-smaller masses. Naively one m...
We present results from the largest numerical simulation of star formation to resolve the fragmentat...
Our first aim is to calculate the minimum mass for Primary Fragmentation in a variety of potential s...
It is estimated that ∼ 60 % of all stars (including brown dwarfs) have masses below 0. 2 M⊙. Current...
The gravitational collapse of a primordial cloud does differ of the gravitational collapse of normal...
In turbulent fragmentation, star formation occurs in condensations created by converging flows. The ...
In turbulent fragmentation, star formation occurs in condensations created by converging flows. The ...
We present a new analysis of the minimum mass for star formation, based on opacity-limited fragmenta...
We present a new analysis of the minimum mass for star formation, based on opacity-limited fragmenta...
We present a new analysis of the minimum mass for star formation, based on opacity-limited fragment...
We present a new analysis of the minimum mass for star formation, based on opacity-limited fragment...
We present a new analysis of the minimum mass for star formation, based on opacity-limited fragmenta...
Context.The minimum mass for star formation is a critical parameter with profound astrophysical, cos...
Context.The minimum mass for star formation is a critical parameter with profound astrophysical, cos...
Theory and simulations suggest that it is possible to form low mass stars via disc fragmentation.The...
As star-forming clouds collapse, the gas within them fragments to ever-smaller masses. Naively one m...
We present results from the largest numerical simulation of star formation to resolve the fragmentat...
Our first aim is to calculate the minimum mass for Primary Fragmentation in a variety of potential s...
It is estimated that ∼ 60 % of all stars (including brown dwarfs) have masses below 0. 2 M⊙. Current...
The gravitational collapse of a primordial cloud does differ of the gravitational collapse of normal...
In turbulent fragmentation, star formation occurs in condensations created by converging flows. The ...
In turbulent fragmentation, star formation occurs in condensations created by converging flows. The ...
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