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Titlebook: Science with the Atacama Large Millimeter Array:; A New Era for Astrop Rafael Bachiller,José Cernicharo Conference proceedings 2008 Springe

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發(fā)表于 2025-3-28 14:44:03 | 只看該作者
42#
發(fā)表于 2025-3-28 22:49:12 | 只看該作者
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發(fā)表于 2025-3-29 01:05:20 | 只看該作者
44#
發(fā)表于 2025-3-29 04:49:55 | 只看該作者
,High-resolution mm interferometry and the search for?massive?protostellar disks: the case of Cep-A ually the result of the superposition of multiple hot-core-type objects, at least one of them ejecting an outflow at a small angle with respect to the line of sight. Together with the well-known large-scale outflow ejected by HW2, this setup makes for a very complex spatial and kinematic picture.
45#
發(fā)表于 2025-3-29 09:23:31 | 只看該作者
SMA observations of the magnetic fields around a low-mass protostellar system,undred AU; gravity has overcome magnetic support and the magnetic field traces a clear hourglass shape. The magnetic field is substantially more important than turbulence in the evolution of the system and the initial misalignment of the magnetic and spin axes may have been important in the formation of the binary system.
46#
發(fā)表于 2025-3-29 14:20:30 | 只看該作者
47#
發(fā)表于 2025-3-29 15:41:31 | 只看該作者
High-mass star forming regions: An ALMA view,massive star formation. The impact of this new generation instrument will range from establishing the mass function of pre-stellar cores inside IR-dark clouds, to investigating the kinematics of the gas from which OB stars are built up, to assessing or ruling out the existence of circumstellar accretion disks in these objects.
48#
發(fā)表于 2025-3-29 19:45:00 | 只看該作者
49#
發(fā)表于 2025-3-30 01:32:10 | 只看該作者
50#
發(fā)表于 2025-3-30 08:00:59 | 只看該作者
ALMA capabilities for observations of continuum emission,ALMA’s sensitivity for continuum measurements is increased with the added feature of an 8 GHz instantaneous bandwidth. Taken together, these four factors provide unparalleled sensitivity in the millimeter/submillimeter wavelength range. With its great sensitivity and angular resolution, ALMA will tr
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