High-resolution polarimetry of Parsamian 21: Revealing the structure of an edge-on FU Ori disc

Monthly Notices of the Royal Astronomical Society

Volumn 383, Issue 3, 2008, Pages 1015-1028

  Kospal A ^a   Abraham P ^a   Apai, D ^b,c   Ardila, D R ^d   Grady, C A ^e   Henning, Th ^f   Juhasz A ^f   Miller, D W ^g   Moor A ^a  

^a INSTITUTE OF EXPERIMENTAL MEDICINE   (Hungary)

^b UNIVERSITY OF ARIZONA   (United States)

^c NASA AMES RESEARCH CENTER   (United States)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

^f MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^g UNIVERSITY OF LOUISVILLE   (United States)

Author keywords

Circumstellar matter; Infrared: stars; Stars: individual: Parsamian 21; Stars: pre main sequence; Techniques: polarimetric

Indexed keywords

ADAPTIVE OPTICS; CAMERAS; ELLIPSOMETRY; INFRARED DEVICES; PHOTOMETRY; POLARIMETERS; SPACE TELESCOPES; SPECTROGRAPHS; STARS;

CIRCUMSTELLAR MATTERS; HIGH RESOLUTION POLARIMETRY; HIGH SPATIAL RESOLUTION; HUBBLE SPACE TELESCOPES; INFRARED: STAR; NEAR INFRARED; STAR: INDIVIDUAL: PARSAMIAN 21; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: PRE-MAIN SEQUENCE; TECHNIQUES: POLARIMETRIC;

SPECTROMETERS;

EID: 38949096050     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12557.x     Document Type: Article

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