Abstract
ABSTRACT The radial velocities of γ1 Vel suggest that we are dealing with a spectroscopic binary of a period of 1d.482575 The scatter of the velocities is large and there seem to be variations in the velocity distribution at different cycles particularly at the quadrature of maximum positive velocity. A new spectrographic investigation with a very good coverage of a number of different cycles is desirable.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Publications of the Astronomical Society of the Pacific
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
