SIMBAD references

1999A&A...348.1040D - Astronomy and Astrophysics, volume 348, 1040-1051 (1999/8-3)

Astrometric radial velocities. I. Non-spectroscopic methods for measuring stellar radial velocity.

DRAVINS D., LINDEGREN L. and MADSEN S.

Abstract (from CDS):

High-accuracy astrometry permits the determination of not only stellar tangential motion, but also the component along the line-of-sight. Such non-spectroscopic (i.e. astrometric) radial velocities are independent of stellar atmospheric dynamics, spectral complexity and variability, as well as of gravitational redshift. Three methods are analysed: (1) changing annual parallax, (2) changing proper motion and (3) changing angular extent of a moving group of stars. All three have significant potential in planned astrometric projects. Current accuracies are still inadequate for the first method, while the second is marginally feasible and is here applied to 16 stars. The third method reaches high accuracy (<1km/s) already with present data, although for some clusters an accuracy limit is set by uncertainties in the cluster expansion rate.

Abstract Copyright:

Journal keyword(s): methods: data analysis - techniques: radial velocities - astrometry - stars: distances - stars: kinematics - Galaxy: open clusters and associations: general

Simbad objects: 68

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:1999A&A...348.1040D and select 'bookmark this link' or equivalent in the popup menu


2020.01.26-12:27:15

© Université de Strasbourg/CNRS

    • Contact