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1995PASP..107..127W - Publ. Astron. Soc. Pac., 107, 127-131 (1995/February-0)
Star No 1412 in M 4, a post-AGB star with low carbon and enhanced TiO.
WHITMER J.C., BECK-WINCHATZ B., BROWN J.A. and WALLERSTEIN G.
Abstract (from CDS):
We can eliminate most causes for the presence of TiO. These include excess oxygen, excess titanium, a hydrogen deficiency, and excess gas pressure. The best remaining possibility is a reduced boundary temperature due to the absence of line blanketing by the CO and CN molecules. A deficiency in CO blanketing may also explain the higher abundances as derived from ionized lines than from neutral lines because the absence of the ultra-violet CO bands may permet an excess of radiation between 1300 and 1550 A to ionize species such as iron and titanium. Other aspects of non-standard model atmospheres are also discussed qualitatively.
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Simbad objects: 4
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