brown dwarf accretion: nonconventional star formation over very long timescales
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ID: 138673
2005
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Abstract
We investigate the process of accretion of interstellar gas by the Galactic population of brown dwarfs over very long timescales typical for physical eschatology. In particular, we use the classical Hoyle-Lyttleton-Bondi accretion model to investigate the rate at which brown dwarfs collect enough additional mass to become red dwarfs, accretion-induced changes in the mass function of the low- mass objects, and the corresponding accretion heating of brown dwarfs. In addition, we show how we can make the definition of the final mass function for stellar objects more precise.
| Reference Key |
m.2005serbianbrown
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| Authors | ;Ćirković Milan M. |
| Journal | saner 2019 - proceedings of the 2019 ieee 26th international conference on software analysis, evolution, and reengineering |
| Year | 2005 |
| DOI |
10.2298/SAJ0571011C
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