The upper mass limit for white dwarf formation as derived from the stellar content of the Hyades cluster

Details The upper mass limit for white dwarf formation as derived from the stellar content of the Hyades cluster The upper mass limit for white dwarf formation as derived from the stellar content of the Hyades cluster

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196l.121v&link_type=gif

Astrophysical Journal, vol. 196, Mar. 15, 1975, pt. 2, p. L121-L123.

Astronomy and Astrophysics

Astrophysics

47

Star Clusters, Stellar Evolution, Stellar Mass, White Dwarf Stars, Astrophysics, Main Sequence Stars, Pulsars, Star Distribution

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