Journal
RESEARCH IN ASTRONOMY AND ASTROPHYSICS
Volume 11, Issue 3, Pages 335-344Publisher
NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
DOI: 10.1088/1674-4527/11/3/007
Keywords
planetary systems: formation; techniques: high angular resolution
Categories
Funding
- Ministry of Education, Culture, Sports, Science and Technology (MEXT), Japan
- [16740256]
Ask authors/readers for more resources
We conducted a near-infrared imaging survey of 11 young dwarfs in the Pleiades cluster using the Subaru Telescope and the near-infrared coronagraph imager. We found ten faint point sources, with magnitudes as faint as 20 mag in the K-band, with around seven dwarfs. Comparison with the Spitzer archive images revealed that a pair of the faint sources around V 1171 Tau is very red in infrared wavelengths, which indicates very low-mass young stellar objects. However, the results of our follow-up proper motion measurements implied that the central star and the faint sources do not share common proper motions, suggesting that they are not physically associated.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available