Fig. 2 from The Mass of the Candidate Exoplanet Companion to HD 33636 from Hubble Space Telescope Astrometry and High‐Precision Radial Velocities

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

The Mass of the Candidate Exoplanet Companion to HD 33636 from Hubble Space Telescope Astrometry and High‐Precision Radial Velocities

Authors: Jacob L. Bean, Barbara E. McArthur, G. Fritz Benedict, Thomas E. Harrison, Dmitry Bizyaev, Edmund Nelan, and Verne V. Smith

Bean et al. 2007 The Astronomical Journal 134 749.

Provider: AAS Journals

Caption: Fig. 2.

Right ascension (α) and declination (δ) components of HD 33636’s perturbation orbit as a function of time (symbols) and the best fit (dashed line) from the simultaneous modeling of the radial velocities and astrometry. The dots represent the individual observations, and the circles represent per epoch (single HST orbit) normal points consisting of 2–4 individual observations.

Other Images in This Article

Copyright and Terms & Conditions