Classification of intrinsic variables. VI - Ultrashort-period, very small amplitude B-type variables

Details Classification of intrinsic variables. VI - Ultrashort-period, very small amplitude B-type variables Classification of intrinsic variables. VI - Ultrashort-period, very small amplitude B-type variables

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...198..131e&link_type=abstract

Astrophysical Journal, vol. 198, May 15, 1975, pt. 1, p. 131-138.

Astronomy and Astrophysics

Astrophysics

5

B Stars, Cepheid Variables, Luminous Intensity, Stellar Evolution, Variable Stars, Binary Stars, Brightness Discrimination, Radial Velocity, Spectroscopic Analysis, Star Clusters, Stellar Mass

Scientific paper

These very young disk-population variables are found to be distributed in a very narrow instability strip, extending from M(bol) = -9 mag to -3 mag and including stars with a range of at least 25 to 5 solar masses. Some new variables, for which periods are not yet available, are suggested as possibly filling the existing gaps in the luminosity distribution and extending the instability region to still lower masses.

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