• Fulltext


        Click here to view fulltext PDF

      Permanent link:

    • Keywords


      stars, spectroscopic binaries; stars, radial velocities; stars, individual

    • Abstract


      A new radial velocity study has been made of the highly eccentric, early-type binary BD -1° 1004 using spectra from the Kavalur Observatory. All available archival material has also been reexamined. An attempt has been made to correct for line ‘dragging’ by the secondary spectrum to improve the fit of the observed data to the orbital solutions. It is found that an earlier suggestion of apsidal regression is still possible although ω is probably constant within the errors. There remain problems and inconsistencies with other orbital elements, in particular K1 and γ

    • Author Affiliations


      N. Kameswara Rao1 B. N. Ashoka1 2 C. Lloyd3 C. D. Pike3 D. J. Stickland3

      1. Indan Institute of Astrophysics, Bangalore - 560034
      2. ISRO Satellite Centre, Bangalore - 560017
      3. Rutherford Appleton Laboratory, Chilton, UK
    • Dates

  • Journal of Astrophysics and Astronomy | News

    • Continuous Article Publication

      Posted on January 27, 2016

      Since January 2016, the Journal of Astrophysics and Astronomy has moved to Continuous Article Publishing (CAP) mode. This means that each accepted article is being published immediately online with DOI and article citation ID with starting page number 1. Articles are also visible in Web of Science immediately. All these have helped shorten the publication time and have improved the visibility of the articles.

    • Editorial Note on Continuous Article Publication

      Posted on July 25, 2019

      Click here for Editorial Note on CAP Mode

© 2021-2022 Indian Academy of Sciences, Bengaluru.