Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...18510408g&link_type=abstract
American Astronomical Society, 185th AAS Meeting, #104.08; Bulletin of the American Astronomical Society, Vol. 26, p.1489
Astronomy and Astrophysics
Astronomy
Scientific paper
We found unexpected spectral characteristics in a set of field horizontal branch stars with spectral types near A0. They showed Balmer line wings that were broad and characteristic of high gravity stars, and further, one third of the FHB stars appeared to have normal metal line strengths despite low m_1 photometric indices. To find out whether the horizontal branch stars in actual clusters show the same characteristics, we have obtained spectra of stars in M3 and in M13. Initial results of classifying these stars support our earlier findings for the FHB stars. We present some atmospheric modelling as our first attempt to understand the parameters of this kind of near-A0, horizontal branch star.
Corbally Christopher J.
Gray Richard O.
Hill James M.
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