SIMBAD references

2007ApJ...666..378M - Astrophys. J., 666, 378-392 (2007/September-1)

The chemical compositions of the type II Cepheids - The BL Herculis and W Virginis variables.

MAAS T., GIRIDHAR S. and LAMBERT D.L.

Abstract (from CDS):

Abundance analyses from high-resolution optical spectra are presented for 19 type II Cepheids in the Galactic field. The sample includes both short-period (BL Her) and long-period (W Vir) stars. This is the first extensive abundance analysis of these variables. The C, N, and O abundances with similar spreads for the BL Her and W Vir show evidence for an atmosphere contaminated with 3α process and CN-cycling products. A notable anomaly of the BL Her stars is an overabundance of Na by a factor of about 5 relative to their presumed initial abundances. This overabundance is not seen in the W Vir stars. The abundance anomalies running from mild to extreme in W Vir stars but not seen in the BL Her stars are attributed to dust-gas separation that provides an atmosphere deficient in elements of high condensation temperature, notably, Al, Ca, Sc, Ti, and s-process elements. Such anomalies have previously been seen among RV Tau stars which represent a long-period extension of the variability enjoyed by the type II Cepheids. Comments are offered on how the contrasting abundance anomalies of BL Her and W Vir stars may be explained in terms of the stars' evolution from the blue horizontal branch.

Abstract Copyright:

Journal keyword(s): Stars: Abundances - Stars: Variables: Other

Simbad objects: 34

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2021.04.13-07:31:21

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