Constraining the accretion rate onto Sagittarius A * using linear polarization

Eliot Quataert, Andrei Gruzinov

    Research output: Contribution to journalArticlepeer-review


    Two possible explanations for the low luminosity of the supermassive black hole at the center of our Galaxy are (1) an accretion rate of the order of the canonical Bondi value (∼10-5 M yr-1) but a very low radiative efficiency for the accreting gas or (2) an accretion rate much less than the Bondi rate. Both models can explain the broadband spectrum of the Galactic center. We show that they can be distinguished using the linear polarization of synchrotron radiation. Accretion at the Bondi rate predicts no linear polarization at any frequency because of Faraday depolarization. Low accretion rate models, on the other hand, have much lower gas densities and magnetic field strengths close to the black hole; polarization may therefore be observable at high frequencies. If confirmed, a recent detection of linear polarization from Sgr A* at ≳ 150 GHz argues for an accretion rate of ∼10-8 M yr-1, much less than the Bondi rate. This test can be applied to other low-luminosity galactic nuclei.

    Original languageEnglish (US)
    Pages (from-to)842-846
    Number of pages5
    JournalAstrophysical Journal
    Issue number2 PART 1
    StatePublished - Dec 20 2000


    • Accretion, accretion disks
    • Galaxy: center
    • Polarization

    ASJC Scopus subject areas

    • Astronomy and Astrophysics
    • Space and Planetary Science


    Dive into the research topics of 'Constraining the accretion rate onto Sagittarius A * using linear polarization'. Together they form a unique fingerprint.

    Cite this