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Infrared Spectroscopy of Symbiotic Stars. V. First Orbits for Three S-Type Systems: Henize 2-173, CL Scorpii, and AS 270

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dc.contributor.authorFekel, Francis C
dc.contributor.authorHinkle, Kenneth H
dc.contributor.authorJoyce, Richard R
dc.contributor.authorWood, Peter R
dc.contributor.authorLebzelter, Thomas
dc.date.accessioned2015-12-07T22:18:43Z
dc.date.issued2007
dc.date.updated2015-12-07T08:23:58Z
dc.description.abstractInfrared radial velocities have been used to compute first orbits of the M giants in three southern S-type symbiotic systems. Of the three, Hen 2-173 has the longest orbital period, 911 days, and also has a noncircular orbit with an eccentricity of 0.21.
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/18948
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Binaries: symbiotic; Infrared: stars; Stars: individual (AS 270, CL Scorpii, Henize 2-173); Stars: late-type
dc.titleInfrared Spectroscopy of Symbiotic Stars. V. First Orbits for Three S-Type Systems: Henize 2-173, CL Scorpii, and AS 270
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage25
local.bibliographicCitation.startpage17
local.contributor.affiliationFekel, Francis C, Tennessee State University
local.contributor.affiliationHinkle, Kenneth H, National Optical Astronomy Observatory
local.contributor.affiliationJoyce, Richard R, National Optical Astronomy Observatory
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLebzelter, Thomas, University of Vienna
local.contributor.authoruidWood, Peter R, u7900259
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4362859xPUB6
local.identifier.citationvolume133
local.identifier.doi10.1086/509133
local.identifier.scopusID2-s2.0-33846492997
local.type.statusPublished Version

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