Show simple item record

dc.contributor.authorKuznetsov, M. K.
dc.contributor.authorPavlenko, Ya. V.
dc.contributor.authorPinfield, D.J.
dc.contributor.authorJones, H.R.A.
dc.identifier.citationKuznetsov , M K , Pavlenko , Y V , Pinfield , D J & Jones , H R A 2012 , ' Physical parameters of the binary star CM draconis components ' , Kinematics and Physics of Celestial Bodies , vol. 28 , no. 3 , pp. 137-141 .
dc.identifier.otherPURE: 961811
dc.identifier.otherPURE UUID: 3e3f343a-7398-497b-9f4b-846f52c8827f
dc.identifier.otherWOS: 000305689700005
dc.identifier.otherScopus: 84862905592
dc.description.abstractSpectra of the eclipsing binary star CM Dra consisting of two M dwarfs are discussed in detail. High-resolution echelle spectra (R = 47000) obtained using the 4.2 m William Hershel telescope are used. The temperatures and metallicities of both components in the binary system are determined using the stellar spectra simulation: T = 3100 +/- 100 K, logg = 5.0 +/- 0.2, [M/H] = -0.5 +/- 0.2 dex. The estimated values are in good agreement with the results obtained by other researchers.en
dc.relation.ispartofKinematics and Physics of Celestial Bodies
dc.titlePhysical parameters of the binary star CM draconis componentsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review

Files in this item


There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record