Spiral structure parameters in the solar neighbourhood

Details Spiral structure parameters in the solar neighbourhood Spiral structure parameters in the solar neighbourhood

2000-10-25

arxiv.org/abs/astro-ph/0010520v1

Astronomy and Astrophysics

Astrophysics

4 pages, no figures, LaTex, uses crckapb.sty. To appear in the Proceedings of the IV Scientific Meeting of the Sociedad Espano

Scientific paper

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.

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