Strong linear polarization of V4332 Sagittarii: A dusty disc geometry (research note)

Astronomy and Astrophysics

Volumn 527, Issue 10, 2011, Pages

  Kaminski T ^a,b   Tylenda, R ^a  

^a NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^b MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

circumstellar matter; polarization; scattering; stars: individual: V4332 Sagittarii; stars: late type; stars: peculiar

Indexed keywords

CIRCUMSTELLAR MATTERS; DUST GRAINS; EMISSION FEATURES; LINEAR POLARIZATION; LINEARLY POLARIZED; OPTICAL LIGHT; STARS: INDIVIDUAL: V4332 SAGITTARII; STARS: LATE-TYPE; STARS: PECULIAR;

DUST; POLARIZATION; SCATTERING;

STARS;

EID: 79551569977     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015950     Document Type: Article

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