Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Branham, Richard Lacy | - |
| dc.date | 2018-11-01T18:02:16Z | - |
| dc.date | 2018-11-01T18:02:16Z | - |
| dc.date | 2017-02 | - |
| dc.date | 2018-10-23T14:41:03Z | - |
| dc.date.accessioned | 2019-04-29T15:42:05Z | - |
| dc.date.available | 2019-04-29T15:42:05Z | - |
| dc.date.issued | 2017-02 | - |
| dc.identifier | Branham, Richard Lacy; The distance to the Galactic center determined by G, K, and M stars; Springer; Astrophysics And Space Science; 362; 2; 2-2017; 1-6 | - |
| dc.identifier | 0004-640X | - |
| dc.identifier | http://hdl.handle.net/11336/63461 | - |
| dc.identifier | CONICET Digital | - |
| dc.identifier | CONICET | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/299903 | - |
| dc.description | The distance from the Sun to the center of the Galaxy R0 remains a fundamental parameter for Galactic structure. This study uses 105,275 G, K, and M stars of all luminosity classes with position, parallax, and proper motion taken from the Hipparcos catalog and radial velocities from the Wilson and Strasbourg Data Center catalogs. The nonlinear kinematical equations of condition are solved by the Nelder-Mead simplex algorithm and give R0=7.64±0.09kpc. At a confidence level of 90 % one can assert the randomness of the residuals and shows that the kinematical model yields satisfactory results. | - |
| dc.description | Fil: Branham, Richard Lacy. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Argentino de Nivología, Glaciología y Ciencias Ambientales. Provincia de Mendoza. Instituto Argentino de Nivología, Glaciología y Ciencias Ambientales. Universidad Nacional de Cuyo. Instituto Argentino de Nivología, Glaciología y Ciencias Ambientales; Argentina | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | Springer | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1007/s10509-017-3015-1 | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs10509-017-3015-1 | - |
| dc.rights | info:eu-repo/semantics/restrictedAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
| dc.source | reponame:CONICET Digital (CONICET) | - |
| dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
| dc.source | instacron:CONICET | - |
| dc.source.uri | http://hdl.handle.net/11336/37288 | - |
| dc.subject | GALAXY: DYNAMICS AND KINEMATICS | - |
| dc.subject | METHODS: DATA ANALYSIS | - |
| dc.subject | NUMERICAL | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | The distance to the Galactic center determined by G, K, and M stars | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| Aparece en las colecciones: | CONICET | |
Ficheros en este ítem:
No hay ficheros asociados a este ítem.