Please use this identifier to cite or link to this item:
https://hdl.handle.net/2445/170928
Title: | Spiral structure parameters in the solar neighbourhood |
Author: | Fernández, D. Luri Carrascoso, Xavier Figueras Siñol, Francesca Torra Roca, Jorge |
Keywords: | Astrofísica Astrophysics |
Issue Date: | 25-Oct-2000 |
Publisher: | Springer Science + Business Media |
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. |
Note: | Versió postprint del document publicat a: https://doi.org/10.1007/978-94-017-1776-2_41 |
It is part of: | Astrophysics and Space Science, 2000, p. 173-176 |
URI: | https://hdl.handle.net/2445/170928 |
Related resource: | https://doi.org/10.1007/978-94-017-1776-2_41 |
ISSN: | 0004-640X |
Appears in Collections: | Articles publicats en revistes (Física Quàntica i Astrofísica) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
173493.pdf | 61.78 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.