The spectroscopic orbit of HD 128220

Details The spectroscopic orbit of HD 128220 The spectroscopic orbit of HD 128220

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.226..249h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 226, May 1, 1987, p. 249-256.

Astronomy and Astrophysics

Astronomy

13

Binary Stars, O Stars, Stellar Evolution, Stellar Orbits, Subdwarf Stars, Astronomical Models, Stellar Mass, Stellar Spectra, Stellar Winds

Scientific paper

HD 128220 is a double-lined binary containing a subdwarf O star. A new orbital solution is presented, based principally on IUE spectroscopy. The implications of the solution for the physical parameters of the subdwarf are discussed, with the results that MOsin3i = 1.6±0.7 M_sun;; ROsin3/2i = 1.2±0.4 R_sun;; and log(LOsin3i/L_sun;) = 3.6±0.3.

Affiliated with

Also associated with

No associations

Rating

The spectroscopic orbit of HD 128220 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 The spectroscopic orbit of HD 128220, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spectroscopic orbit of HD 128220 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-859238