CO Emission from Disks around AB Aurigae and HD 141569: Implications for Disk Structure and Planet Formation Timescales
- 1 May 2003
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 588 (1), 535-544
- https://doi.org/10.1086/373987
Abstract
No abstract availableThis publication has 40 references indexed in Scilit:
- CO and H3+ in the protoplanetary disk around the star HD141569Nature, 2002
- High‐Resolution 4.7 Micron Keck/NIRSPEC Spectra of Protostars. I. Ices and Infalling Gas in the Disk of L1489 IRSThe Astrophysical Journal, 2002
- Passive Irradiated Circumstellar Disks with an Inner HoleThe Astrophysical Journal, 2001
- Carbon Monoxide Production and Excitation in Comet C/1995 O1 (Hale-Bopp): Isolation of Native and Distributed CO SourcesIcarus, 2001
- Evidence for Residual Material in Accretion Disk Gaps: CO Fundamental Emission from the T Tauri Spectroscopic Binary DQ TauriThe Astrophysical Journal, 2001
- Spectral Energy Distributions of Passive T Tauri and Herbig Ae Disks: Grain Mineralogy, Parameter Dependences, and Comparison withInfrared Space ObservatoryLWS ObservationsThe Astrophysical Journal, 2001
- Detection of Extended Thermal Infrared Emission around the Vega-like Source HD 141569The Astrophysical Journal, 2000
- Spectral Energy Distributions of Passive T Tauri Disks: InclinationThe Astrophysical Journal, 1999
- High-resolution spectroscopy of Vega-like stars -- I. Effective temperatures, gravities and photospheric abundancesMonthly Notices of the Royal Astronomical Society, 1997
- The Gas Drag Effect on the Elliptic Motion of a Solid Body in the Primordial Solar NebulaProgress of Theoretical Physics, 1976