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Polarized light from Sagittarius A(star) in the near-infrared K-s-band

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    0444413 - ASÚ 2016 RIV FR eng J - Journal Article
    Shahzamanian, B. - Eckart, A. - Valencia-S, M. - Witzel, G. - Zamaninasab, M. - Sabha, N. - García-Marín, M. - Karas, Vladimír - Karssen, G. - Borkar, A. - Dovčiak, Michal - Kunneriath, Devaky - Bursa, Michal - Buchholz, R. M. - Moultaka, J. - Straubmeier, C.
    Polarized light from Sagittarius A(star) in the near-infrared K-s-band.
    Astronomy & Astrophysics. Roč. 576, April (2015), A20/1-A20/18. ISSN 0004-6361. E-ISSN 1432-0746
    Grant - others:EU(XE) COST Action MP0905; EU(XE) COST action MP1104
    Institutional support: RVO:67985815
    Keywords : black hole physics * accretion disks * galaxy center
    OECD category: Astronomy (including astrophysics,space science)
    Impact factor: 5.185, year: 2015

    We present a statistical analysis of polarized near-infrared light from Sgr A*, the radio source associated with the supermassive black hole at the center of the Milky Way. The observations were carried out using the adaptive optics instrument NACO at the VLT UT4 in the infrared K-s-band from 2004 to 2012.
    Permanent Link: http://hdl.handle.net/11104/0246942

     
     
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