Possible iron abundance variations among superficially normal A stars

From National Research Council Canada

DOIResolve DOI: https://doi.org/10.1086/159722
AuthorSearch for: 1; Search for: ; Search for: 1; Search for:
Affiliation
  1. National Research Council of Canada. NRC Herzberg Institute of Astrophysics
FormatText, Article
SubjectA stars; abundance; early stars; iron; peculiar stars; stellar rotation; stellar spectra; B stars; interstellar matter; late stars: radial velocity
Abstract
Publication date
PublisherAmerican Astronomical Society
IOP Publishing
In
LanguageEnglish
Peer reviewedYes
NRC numberNRCC 21188
NPARC number21275048
Export citationExport as RIS
Report a correctionReport a correction (opens in a new tab)
Record identifierf2b7854a-779b-423a-8e70-e7eaea45f5cc
Record created2015-05-06
Record modified2020-03-13
Date modified: