Interferometric Observations of the T Tauri Stars in the MBM 12 Cloud
arXiv:astro-ph/0302472 · doi:10.1086/374881
Abstract
We have carried out a millimeter interferometric continuum survey toward 7 YSOs in the MBM 12 cloud. Thermal emissions associated with 2 YSOs were detected above the 3- level at 2.1 mm, and one also showed a 1.3 mm thermal emission. Another object was marginally detected at 2.1 mm. Spectral energy distributions of the YSOs are well fitted by a simple power-law disk model. Masses of the circumstellar disks are estimated to be an order of $0.05 M_{\sun}$. The circumstellar disks in the MBM 12 cloud have properties in common with the disks in nearby star-forming regions, in terms of disk parameters such as a disk mass, as well as an infrared excess.
arXiv comment9 pages, 3 figures, accepted by ApJ Letters
References in corpus (5)
- Spherically symmetric model atmospheres for low mass pre-Main Sequence stars with effective temperatures between 2000 and 6800 K
- On the MBM12 Young Association
- Protoplanetary Disks in the Nearest Star-Forming Cloud: Mid-Infrared Imaging and Optical Spectroscopy of MBM 12 Members
- Adaptive optics imaging of the MBM 12 association
- Millimeter-wave Searches for Cold Dust and Molecular Gas around T Tauri Stars in MBM 12
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- An ALMA Continuum Survey of Circumstellar Disks in the Upper Scorpius OB Association
- Distribution of Circumstellar Disk Masses in the Young Cluster NGC 2024
- MBM 12: young protoplanetary discs at high galactic latitude
- High spatial resolution optical imaging of the multiple T Tauri system LkHα 262/LkHα 263
- Detection of Molecular Hydrogen Emission Associated with LkHalpha 264
- Indications for grain growth and mass decrease in cold dust disks around Classical T Tauri stars in the MBM 12 young association
- Outbursts of Young Stellar Objects
- AzTEC 1.1 mm Observations of the MBM12 Molecular Cloud
- A Photometric Study of Stars in the MBM 12 Association