A reappraisal of the gap in the HR diagram of M67

Details A reappraisal of the gap in the HR diagram of M67 A reappraisal of the gap in the HR diagram of M67

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.182..219m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 182, Jan. 1978, p. 219-231.

Astronomy and Astrophysics

Astronomy

23

Binary Stars, Galactic Clusters, Hertzsprung-Russell Diagram, Stellar Evolution, Stellar Models, Convective Flow, Electrophotometry, Stellar Mass, Stellar Spectrophotometry

Scientific paper

Consideration of the effects of unresolved binaries and observational errors, and careful application of the Schwarzschild criterion at the boundary of the convective core, show that the observed HR diagram of M67 can be modeled with stars computed conventionally, i.e., without using convective overshooting. The computed isochrone is used to show that M67 may have a constant mass function.

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