An abundance analysis of Tau Herculis, B5 IV

Details An abundance analysis of Tau Herculis, B5 IV An abundance analysis of Tau Herculis, B5 IV

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.181..667a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 181, Dec. 1977, p. 667-675.

Astronomy and Astrophysics

Astronomy

10

Abundance, Atmospheric Composition, B Stars, Stellar Atmospheres, Stellar Models, Atmospheric Models, Line Spectra, Main Sequence Stars, Tables (Data)

Scientific paper

An abundance analysis of the sharp-lined star Tau Herculis (B5 IV) has
been performed using a fully line-blanketed model atmosphere. The
derived abundances are similar to those of the sun and the normal
main-sequence B stars Iota Her (B3 V) and Nu Cap (B9 V).

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