Spiral structure parameters in the solar neighbourhood
| dc.contributor.author | Fernández, D. | |
| dc.contributor.author | Luri Carrascoso, Xavier | |
| dc.contributor.author | Figueras Siñol, Francesca | |
| dc.contributor.author | Torra Roca, Jorge | |
| dc.date.accessioned | 2020-09-29T10:08:39Z | |
| dc.date.available | 2020-09-29T10:08:39Z | |
| dc.date.issued | 2000-10-25 | |
| dc.date.updated | 2020-09-29T10:08:39Z | |
| dc.description.abstract | Two samples of O- and B-type stars and Cepheids with Hipparcos data have been used to characterize galactic rotation and spiral arm kinematics in the solar neighbourhood. An extensive set of simulations has been performed in order to assess the capabilities of the method and its sensitivity to sample errors and biases in the adopted parameters. | |
| dc.format.extent | 4 p. | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.idgrec | 173493 | |
| dc.identifier.issn | 0004-640X | |
| dc.identifier.uri | https://hdl.handle.net/2445/170928 | |
| dc.language.iso | eng | |
| dc.publisher | Springer Science + Business Media | |
| dc.relation.isformatof | Versió postprint del document publicat a: https://doi.org/10.1007/978-94-017-1776-2_41 | |
| dc.relation.ispartof | Astrophysics and Space Science, 2000, p. 173-176 | |
| dc.relation.uri | https://doi.org/10.1007/978-94-017-1776-2_41 | |
| dc.rights | (c) Springer Science + Business Media, 2000 | |
| dc.rights.accessRights | info:eu-repo/semantics/openAccess | |
| dc.source | Articles publicats en revistes (Física Quàntica i Astrofísica) | |
| dc.subject.classification | Astrofísica | |
| dc.subject.other | Astrophysics | |
| dc.title | Spiral structure parameters in the solar neighbourhood | |
| dc.type | info:eu-repo/semantics/article | |
| dc.type | info:eu-repo/semantics/acceptedVersion |
Fitxers
Paquet original
1 - 1 de 1