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Séminaire du Jeudi 21 Mars 2013

Looking for planets around M dwarfs with adaptive optics direct imaging

Philippe Delorme (IPAG)
Jeudi 21 Mars - 11 h 00
Salle Manuel Forestini - IPAG

To investigate whether formation of large separation planets is correlated with stellar host mass, we systematically imaged young M dwarfs of the solar neigbhourhood with NACO adaptive optic imager at VLT. We applied the latest central star removal technics (ADI, LOCI...) to search for Jupiter mass planets around this sample. We present here what we found and what we did not found after 2 years of survey.

Slides in PDF format

Sous la tutelle de:


Sous la tutelle de:

CNRS Université Grenoble Alpes