CO ROVIBRATIONAL EMISSION AS A PROBE OF INNER DISK STRUCTURE

Journal Article · Tue Dec 20 04:00:00 EST 2011 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/743/2/112· OSTI ID:22004467

Salyk, C ^[1]; Blake, G A ^[2]; Boogert, A C. A. ^[3]; Brown, J M ^[4]

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1. McDonald Observatory, University of Texas at Austin, 1 University Station, C1402, Austin, TX 78712 (United States)
2. Division of Geological and Planetary Sciences, California Institute of Technology, Mail Code 150-21, Pasadena, CA 91125 (United States)
3. California Institute of Technology, Infrared Processing and Analysis Center, Mail Code 100-22, Pasadena, CA 91125 (United States)
4. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

We present an analysis of CO emission lines from a sample of T Tauri, Herbig Ae/Be, and transitional disks with known inclinations in order to study the structure of inner disk molecular gas. We calculate CO inner radii by fitting line profiles with a simple parameterized model. We find that, for optically thick disks, CO inner radii are strongly correlated with the total system luminosity (stellar plus accretion) and consistent with the dust sublimation radius. Transitional disk inner radii show the same trend with luminosity, but are systematically larger. Using rotation diagram fits, we derive, for classical T Tauri disks, emitting areas consistent with a ring of width {approx}0.15 AU located at the CO inner radius; emitting areas for transitional disks are systematically smaller. We also measure lower rotational temperatures for transitional disks, and disks around Herbig Ae/Be stars, than for those around T Tauri stars. Finally, we find that rotational temperatures are similar to, or slightly lower than, the expected temperature of blackbody grains located at the CO inner radius, in contrast to expectations of thermal decoupling between gas and dust.

• OSTI ID: 22004467
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 743; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
DUSTS
LUMINOSITY
PROTOPLANETS
ROTATION
SUBLIMATION
T TAURI STARS