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Elemental abundance analyses with DAO spectrograms – XXIII. The superficially normal stars 28 And (A7 III) and 99 Her (F7 V)
Author(s) -
Adelman Saul J.,
Caliskan Hulya,
Kocer Dursun,
Cay Ipek H.,
Gokmen Tektunali H.
Publication year - 2000
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2000.03577.x
Subject(s) - microturbulence , physics , astrophysics , stars , abundance (ecology) , spectral line , variable star , metal , star (game theory) , astronomy , chemistry , fishery , biology , organic chemistry
Elemental abundances of 28 And (A7 III) and 99 Her (F7 V), which have modest rotational velocities, are derived in a manner consistent with previous studies in this series of papers. The values for 28 And, a δ Scuti variable, show that it is slightly metal‐poor, but not a classical Am star. 99 Her, which is somewhat more metal‐poor, has a rather small microturbulence for its spectral type.

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