Near-infrared Coronagraphy of the GG Tauri A binary system

Publications of the Astronomical Society of Japan

Volumn 54, Issue 6, 2002, Pages 963-967

  Itoh, Yoichi ^a   Tamura, Motohide ^b   Hayashi, Saeko S ^b   Oasa, Yumiko ^c   Fukagawa, Misato ^d   Kaifu, Norio ^b   Suto, Hiroshi ^b   Murakawa, Koji ^b   Doi, Yoshiyuki ^b   Ebizuka, Noboru ^e   Naoi, Takahiro ^d   Takami, Hideki ^b   Takato, Naruhisa ^b   Gaessler, Wolfgang ^b   Kanzawa, Tomio ^b   Hayano, Yutaka ^b   Kamata, Yukiko ^b   Saint Jacques, David ^b   Iye, Masanori ^b  

^a KOBE UNIVERSITY   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^d UNIVERSITY OF TOKYO   (Japan)

^e INST OF PHYS AND CHEMICAL RESEARCH   (Japan)

Author keywords

Stars: individual (GG Tauri); Stars: pre main sequence; Techniques: high angular resolution

Indexed keywords

ADAPTIVE OPTICS; INFRARED DEVICES; INFRARED IMAGING; SYSTEMS (METALLURGICAL);

BINARY SYSTEMS; CORONAGRAPHY; HIGH ANGULAR RESOLUTIONS; NEAR INFRARED; NEAR- INFRARED IMAGES; NEAR-INFRARED; STAR: INDIVIDUAL (GG TAURI); STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: PRE-MAIN SEQUENCE; TECHNIQUES: HIGH ANGULAR RESOLUTIONS;

STARS;

EID: 0036934651     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/54.6.963     Document Type: Article

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