Research Project
Grant-in-Aid for Research Activity Start-up
It is essential to clarify the mechanism of protoplanetary disk dispersal for understanding planet formation processes. We observed star-forming regions in higher and lower metallicity environments with Subaru 8.2m telescope and found the metallicity dependence of disk lifetime : the longer lifetime in higher metallicity environments. Our results suggest that photoevaporation by FUV and/or X-ray is one of the most dominant mechanism in disk dispersal process. We also quantitatively estimated disk lifetime of intermediate-mass stars for the first time and found that the lifetime is about half of that for low-mass stars and that the innermost disk disappears in very short timescale while entire disk disappears almost simultaneously for low-mass stars.
All 2012 2011 2010 Other
All Journal Article (6 results) (of which Peer Reviewed: 4 results) Presentation (5 results) Remarks (5 results)
Publications of the Astronomical Society of Japan
Volume: 63巻、1号
Volume: 63
The Astrophysical Journal Letters
Volume: 723巻、1号 Issue: 1 Pages: L113-L116
10.1088/2041-8205/723/1/l113
http://adsabs.harvard.edu/abs/2011PASJ.63L.1K
Proc. SPIE
Volume: 7739 Pages: 77394G-77394G
10.1117/12.856631
The Astrophysical Journal
Volume: 723
Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
Volume: 7739
http://ngm.nationalgeographic.com/2010/12/milky-way/croswell-text/3
http://nng.nikkeibp.co.jp/nng/magazine/1012/feature02/