SIMBAD references

1999A&A...350..859S - Astronomy and Astrophysics, volume 350859-864 (1999/10-3)

A comparative high-resolution spectroscopic study of the Hyades giants γ Tauri and ε Tauri.

SMITH G.

Abstract (from CDS):

Spectra of the Hyades K0 giants γ Tau and ε Tau in the regions 5852-5864Å and 6145-6176Å have been recorded at high resolution and with signal/noise in the range 150-250. A critical comparison reveals that, although nearly all lines in the observed regions have a similar depth, lines of ε Tau are broader by about 10% than those of γ Tau. An LTE analysis indicates that slightly higher turbulent broadening in ε Tau can account for the observed differences in line-width. Study of two particularly temperature sensitive features confirms earlier observations that the effective temperature of ε Tau is less than that of γ Tau and determines the temperature difference to be 80±20K.

Abstract Copyright: ∼

Journal keyword(s): stars: abundances - stars: fundamental parameters - stars: individual: γ Tau - stars: individual: ε Tau - stars: late-type

Simbad objects: 8

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