Near-IR speckle imaging of massive young stellar objects
arXiv:astro-ph/0407079 · doi:10.1051/0004-6361:20034438
Abstract
We present near-IR speckle images of 21 massive Young Stellar Objects (YSOs) associated with outflows. The aim of this study is to search for sub-arcsecond reflection nebulae associated with the outflow cavity. We find that 6 of the massive YSOs show a conical nebula which can be interpreted in terms of reflected light from the dusty walls of the outflow cavity. In all cases, the small scale structures seen in our images are compared with outflow indicators found in the literature. No clear correlation is found between the presence of the reflection nebulosity and any property such as degree of embeddedness. We also note that 3 of the sources show close companions, one of them belonging also to the sample with conical nebula.
17 pages, 16 figures, accepted for publication in A&A
References in corpus (13)
- 2-D Radiative Transfer in Protostellar Envelopes: I. Effects of Geometry on Class I Sources
- HST/STIS Spectroscopy of the Optical Outflow from DG Tau: Indications for Rotation in the Initial Jet Channel
- Radiation driven winds from luminous accretion disks
- Collapse of Rotating Magnetized Molecular Cloud Cores and Mass Outflows
- The Population of the Galactic Plane as Seen by MSX
- Hydrodynamical Simulations of Jet- and Wind-driven Protostellar Outflows
- A dusty torus around the luminous young star LkHa 101
- Multiple outflows in IRAS 19410+2336
- A Mid-Infrared Study of the Young Stellar Population in the NGC 2024 Cluster
- Imaging the disk around the luminous young star LkHalpha 101 with infrared interferometry
- Visual binaries among high-mass stars - An adaptive optics survey of OB stars in the NGC 6611 cluster
- Outflow collimation in young stellar objects
- Constraints in the circumstellar density distribution of massive Young Stellar Objects
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