Abstract
We present multi-epoch Spitzer Space Telescope observations of the transitional disk LRLL 31 in the 2-3 Myr old star-forming region IC 348. Our measurements show remarkable mid-infrared variability on timescales as short as one week. The infrared continuum emission exhibits systematic wavelength-dependent changes that suggest corresponding dynamical changes in the inner disk structure and variable shadowing of outer disk material. We propose several possible sources for the structural changes, including a variable accretion rate or a stellar or planetary companion embedded in the disk. Our results indicate that variability studies in the infrared can provide important new constraints on protoplanetary disk behavior.
Original language | English (US) |
---|---|
Pages (from-to) | L15-L19 |
Journal | Astrophysical Journal |
Volume | 704 |
Issue number | 1 PART 2 |
DOIs | |
State | Published - 2009 |
Keywords
- Accretion, accretion disks
- Planetary systems: protoplanetary disks
- Stars: pre-main sequence
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science