VLT/NACO adaptive optics imaging of the TY CrA system. A fourth stellar component candidate detected

Astronomy and Astrophysics

Volumn 406, Issue 3, 2003, Pages

  Chauvin, G ^a   Lagrange, A M ^a   Beust, H ^a   Fusco, T ^b   Mouillet, D ^c   Lacombe, F ^d   Pujet, P ^e   Rousset, G ^b   Gendron, E ^d   Conan, J M ^b   Bauduin, D ^d   Rouan, D ^d   Brandner, W ^f   Lenzen, R ^f   Hubin, N ^g   Hartung, M ^f  

^a LABORATOIRE D ASTROPHYSIQUE   (France)

^b ONERA   (France)

^c OBSERVATOIRE MIDI PYRÉNÉES   (France)

^d OBSERVATOIRE DE PARIS   (France)

^e CANADA FRANCE HAWAII TELESCOPE   (United States)

^f MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^g EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Binaries: eclipsing; Circumstellar matter; Stars: low mass; Stars: pre main sequence

Indexed keywords

ADAPTIVE OPTICS; ALGORITHMS; CHROMIUM COMPOUNDS; DUST; GALAXIES; INFRARED IMAGING; OPTICAL SENSORS; PARTICLES (PARTICULATE MATTER); PHOTOMETRY; WAVEFRONTS;

ADAPTIVE OPTICS IMAGING; LOW MASS CIRCUMSTELLAR MATTER; STAR; TRIPLE YOUNG SYSTEM;

CLOUDS;

EID: 0042197586     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030554     Document Type: Letter

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