Spectroastrometry: A new approach to astronomy on small spatial scales

Jeremy Bailey*

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    38 Citations (Scopus)

    Abstract

    The technique of spectroastrometry (measuring the wavelength dependence of the position of an object) provides a means of studying the spatial structure of astronomical sources on scales much smaller than the seeing disk size or the diffraction limit. Despite successful demonstrations in the past, the method does not seem to be widely known. This paper describes techniques used at the Anglo-Australian Telescope to obtain such observations with standard instrumentation, and presents some examples of astronomical results on sources including binary stars and active galactic nuclei. The potential for combining spectroastrometry with interferometry to observe structure on microarcsecond scales is described.

    Original languageEnglish
    Pages (from-to)932-939
    Number of pages8
    JournalProceedings of SPIE - The International Society for Optical Engineering
    Volume3355
    DOIs
    Publication statusPublished - 1998

    Keywords

    • Active galactic nuclei
    • Binary stars
    • Interferometry
    • Pre-main-sequence stars
    • Spectroastrometry

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