Spitzer Observations of Bok Globule B335: Isolated Star Formation Efficiency and Cloud Structure
arXiv:0807.2241 · doi:10.1086/591789
Abstract
We present infrared and millimeter observations of Barnard 335, the prototypical isolated Bok globule with an embedded protostar. Using Spitzer data we measure the source luminosity accurately; we also constrain the density profile of the innermost globule material near the protostar using the observation of an 8.0 um shadow. HHT observations of 12CO 2 --> 1 confirm the detection of a flattened molecular core with diameter ~10000 AU and the same orientation as the circumstellar disk (~100 to 200 AU in diameter). This structure is probably the same as that generating the 8.0 um shadow and is expected from theoretical simulations of collapsing embedded protostars. We estimate the mass of the protostar to be only ~5% of the mass of the parent globule.
15 pages, 17 figures, emulateapj format, accepted for publication in ApJ
References in corpus (6)
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- Models of Rotating Infall for the B335 Protostar
- Intensity-Corrected Herschel Observations of Nearby Isolated Low-Mass Clouds
- JCMT POL-2 and ALMA polarimetric observations of 6000-100 au scales in the protostar B335: linking magnetic field and gas kinematics in observations and MHD simulations
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