SIMBAD references

2001A&A...372..833F - Astronomy and Astrophysics, volume 372, 833-850 (2001/6-4)

Kinematics of young stars. II. Galactic spiral structure.


Abstract (from CDS):

The young star velocity field is analysed by means of a galactic model which takes into account solar motion, differential galactic rotation and spiral arm kinematics. We use two samples of Hipparcos data, one containing O- and B-type stars and another one composed of Cepheid variable stars. The robustness of our method is tested through careful kinematic simulations. Our results show a galactic rotation curve with a classical value of A Oort constant for the O and B star sample (AOB=13.7-13.8km/s/kpc) and a higher value for Cepheids (ACep=14.9-16.9km/s/kpc, depending on the cosmic distance scale chosen). The second-order term is found to be small, compatible with a zero value. The study of the residuals shows the need for a K-term up to a heliocentric distance of 4kpc, obtaining a value K=-(1-3)km/s/kpc. The results obtained for the spiral structure from O and B stars and Cepheids show good agreement. The Sun is located relatively near the minimum of the spiral perturbation potential (ψ=284-20°) and very near the corotation circle. The angular rotation velocity of the spiral pattern was found to be Ωp≃30km/s/kpc.

Abstract Copyright:

Journal keyword(s): Galaxy: kinematics and dynamics - Galaxy: solar neighbourhood - Galaxy: structure - stars: early-type - stars: kinematics - stars: variables: Cepheids

Simbad objects: 7

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2001A&A...372..833F and select 'bookmark this link' or equivalent in the popup menu


© Université de Strasbourg/CNRS

    • Contact