Radial Velocities for 889 Late‐Type Stars
San Francisco State University · University of California, Berkeley · +3 more institutions
Abstract
We report radial velocities for 844 FGKM-type main sequence and subgiant stars and 45 K giants, most of which had either low-precision velocity measurements or none at all. These velocities differ from the standard stars of Udry et al. by 0.035 km/s (RMS) for the 26 FGK standard stars in common. The zero-point of our velocities differs from that of Udry et al.: (V_present - V_Udry) = +0.053 km/s. Thus these new velocities agree with the best known standard stars both in precision and zero-point, to well within 0.1 km/s. Nonetheless, both these velocities and the standards suffer from three sources of systematic error, namely, convective blueshift, gravitational redshift, and spectral type mismatch of the…
Citation impact
- FWCI
- 17.54
- Percentile
- 100%
- References
- 42
Authors
5- DLDavid L. NideverCorresponding
San Francisco State University
- GWGeoffrey W. Marcy
San Francisco State University, University of California, Berkeley
- RPR. Paul Butler
Carnegie Institution for Science, Carnegie Observatories
- DADebra A. Fischer
University of California, Berkeley
- SSSteven S. Vogt
University of California, Santa Cruz
Topics & keywords
- Stars
- Physics
- Astrophysics
- Subgiant
- Radial velocity
- Stellar classification
- Sky
- Spectral line