Variable Stars

Details Variable Stars Variable Stars

Mar 1886

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1886natur..33..440m&link_type=abstract

Nature, Volume 33, Issue 854, pp. 440-441 (1886).

Physics

Scientific paper

IN the last number of NATURE (p. 397) Prof. Seeliger, of Munich, is represented as thinking ``it not improbable that the blazing forth of the Nova may have been due to a collision which caused an enormous development of heat and light.'' It appears to me that the collision hypothesis is not necessary, and that the variability of a star is a physico-chemical consequence of mere cooling. This conclusion is based on considerations relating to the formation of the chemical elements.

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