A model-atmosphere analysis of Ap star HD 26385
Astrophysics and Space Science, ISSN: 0004-640X, Vol: 185, Issue: 2, Page: 237-247
1991
- 2Citations
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
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Metrics Details
- Citations2
- Citation Indexes2
- CrossRef1
Article Description
An abundance analysis using photographic region spectrograms and fully line-blanketed model atmospheres has been performed for the chemically peculiar (CP) star HD 26385. Model parameters were determined from Hγ-profile and photometric data. Its pattern of abundance shows that HD 26385 is typically Ap Si-star. © 1991 Kluwer Academic Publishers.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=20844445699&origin=inward; http://dx.doi.org/10.1007/bf00643191; http://link.springer.com/10.1007/BF00643191; http://link.springer.com/content/pdf/10.1007/BF00643191; http://link.springer.com/content/pdf/10.1007/BF00643191.pdf; http://link.springer.com/article/10.1007/BF00643191/fulltext.html; http://www.springerlink.com/index/10.1007/BF00643191; http://www.springerlink.com/index/pdf/10.1007/BF00643191; https://dx.doi.org/10.1007/bf00643191; https://link.springer.com/article/10.1007/BF00643191
Springer Nature
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