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Astronomy and Astrophysics
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Astronomy and Astrophysics
Article . 2003 . Peer-reviewed
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New spectroscopic binaries among nearby stars

descriptionPublicationkeyboard_double_arrow_right Article 24 Feb 2003Publisher:EDP SciencesJournal:Astronomy & Astrophysics, volume 400, pages 293-296 (issn: 0004-6361, eissn: 1432-0746, Copyright policy )
Authors: J. H. M. M. Schmitt; Swetlana Hubrig; R. Wichmann;

doi: 10.1051/0004-6361:20021915

New spectroscopic binaries among nearby stars

Abstract

In the course of surveying a large number of nearby ( ≈ 50 pc or less) stars for indicators of youth, we have discovered a number of hitherto unknown spectroscopic binaries. Here we present a list of these new binaries with pertinent data. Two of these (HD 143705 and HD 89959) have been observed six times each, and their respective radial velocity curves are discussed.

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    		 16
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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
16
Average
Top 10%
Average
bronze
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