Spatially resolving the inner disk of TW hydrae

Joshua A Eisner, E. I. Chiang, L. A. Hlllenbrand

Research output: Contribution to journalArticle

68 Citations (Scopus)

Abstract

We present Keck Interferometer observations of TW Hya that spatially resolve its emission at 2 μm wavelength. Analyzing these data together with existing K-band veiling and near-infrared photometric measurements, we conclude that the inner disk consists of optically thin, submicron-sized dust extending from ∼4 AU to within 0.06 AU of the central star. The inner disk edge may be magnetospherically truncated. Even if we account for the presence of gas in the inner disk, these small dust grains have survival times against radiation blowout that are orders of magnitude shorter than the age of the system, suggesting continual replenishment through collisions of larger bodies.

Original languageEnglish (US)
JournalAstrophysical Journal
Volume637
Issue number2 II
DOIs
StatePublished - Feb 1 2006
Externally publishedYes

Fingerprint

dust
blowout
interferometer
replenishment
near infrared
collision
extremely high frequencies
wavelength
interferometers
gas
stars
collisions
radiation
gases
wavelengths

Keywords

  • Planetary systems: protoplanetary disks
  • Stars: individual (TW Hydrae)
  • Stars: pre-main-sequence

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Spatially resolving the inner disk of TW hydrae. / Eisner, Joshua A; Chiang, E. I.; Hlllenbrand, L. A.

In: Astrophysical Journal, Vol. 637, No. 2 II, 01.02.2006.

Research output: Contribution to journalArticle

Eisner, Joshua A ; Chiang, E. I. ; Hlllenbrand, L. A. / Spatially resolving the inner disk of TW hydrae. In: Astrophysical Journal. 2006 ; Vol. 637, No. 2 II.
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