| dc.contributor.author | Kuznetsov, M. K. | |
| dc.contributor.author | Pavlenko, Ya. V. | |
| dc.contributor.author | Pinfield, D.J. | |
| dc.contributor.author | Jones, H.R.A. | |
| dc.date.accessioned | 2013-02-11T11:00:19Z | |
| dc.date.available | 2013-02-11T11:00:19Z | |
| dc.date.issued | 2012-05 | |
| dc.identifier.citation | Kuznetsov , 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 . https://doi.org/10.3103/S088459131203004X | |
| dc.identifier.issn | 0884-5913 | |
| dc.identifier.uri | http://hdl.handle.net/2299/9933 | |
| dc.description.abstract | Spectra 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.format.extent | 5 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Kinematics and Physics of Celestial Bodies | |
| dc.title | Physical parameters of the binary star CM draconis components | en |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
| dc.description.status | Peer reviewed | |
| rioxxterms.versionofrecord | 10.3103/S088459131203004X | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
