Application of the Fourier transform for solving and improving spectroscopic binary star orbits

Details Application of the Fourier transform for solving and improving spectroscopic binary star orbits Application of the Fourier transform for solving and improving spectroscopic binary star orbits

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...302..764a&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 302, March 15, 1986, p. 764-766.

Statistics

Computation

Astronomical Spectroscopy, Binary Stars, Computational Astrophysics, Fourier Transformation, Stellar Orbits, Correction, Orbital Elements, Radial Velocity

Scientific paper

A new method of improving a preliminary orbit is found by means of the
corrections of the Fourier coefficients. An application of the method is
made for the systems HD 149240 and 105 Herculis.

Affiliated with

Also associated with

No associations

Rating

Application of the Fourier transform for solving and improving spectroscopic binary star orbits does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Application of the Fourier transform for solving and improving spectroscopic binary star orbits, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Application of the Fourier transform for solving and improving spectroscopic binary star orbits will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1280658