Eruptive Variables

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DOI: 10.4236/jhepgc.2016.22014    1,665 Downloads   2,529 Views  Citations

ABSTRACT

In this paper, a solution of the problem about how a massive star knows that it gets rid of its excess of mass before it can become a white dwarf, a pulsar or a black hole, is proposed. Many astronomers believe that this may take place in the form of a nova and supernova outburst, as well as in the form of a continuous outflow of gas [1].

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Palacios, A. (2016) Eruptive Variables. Journal of High Energy Physics, Gravitation and Cosmology, 2, 155-160. doi: 10.4236/jhepgc.2016.22014.

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