Spiral structure parameters in the solar neighbourhood

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dc.creatorFernandez, D.
dc.creatorLuri, X.
dc.creatorFigueras, F.
dc.creatorTorra, J.
dc.date2000-10-25
dc.date.accessioned2026-07-25T11:25:22Z
dc.descriptionTwo 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.description4 pages, no figures, LaTex, uses crckapb.sty. To appear in the Proceedings of the IV Scientific Meeting of the Sociedad Espanola de Astronomia (SEA)
dc.identifierhttps://arxiv.org/abs/astro-ph/0010520
dc.identifierhttp://arxiv.org/abs/astro-ph/0010520
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/2567
dc.subjectAstrophysics
dc.titleSpiral structure parameters in the solar neighbourhood
dc.typetext

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