CAOSP abstracts, Volume: 49, No.: 3, year: 2019

Abstract: The broadening-function technique was applied to three binaries and a transiting exoplanet. The faint secondary component in IN Vir was detected. BD And was found to be a triple star. The rotational axis of the primary component of α CrB was found to be practically perpendicular to the orbital plane. A transiting planet signature was clearly found in Kelt-7b data.

Full text version of this article in PostScript (600dpi) format compressed by gzip; or in PDF.


Back to:
CAOSP Vol. 49 No. 3 index
CAOSP archive main index
CAOSP main page
Astronomical Institute home page
Valid XHTML 1.0! Valid CSS!

Last update: December 21, 2019