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The Average Magnetic Field Strength in Molecular Clouds: New Evidence of Super-Alfvenic Turbulence
Paolo Padoan, Raul Jimenez, Mika Juvela +1
The magnetic field strength in molecular clouds is a fundamental quantity for theories of star formation. It is estimated by Zeeman splitting measurements in a few dense molecular…
Morphology and kinematics of Lynds 1642
D. Russeil, M. Juvela, K. Lehtinen +2
The high latitude translucent molecular cloud L1642 has been mapped in the J=1-0 and J=2-1 transitions of 12CO, 13CO and C18O using the SEST radio telescope. We have analysed the m…
Photoelectric heating and [CII] cooling in translucent clouds: results for cloud models based on simulations of compressible MHD turbulence
M. Juvela, P. Padoan, R. Jimenez
The photoelectric heating is believed to be the main heating mechanism in cool HI clouds. The heating rate can be estimated through observations of the [CII] line emission, since t…
Submillimeter Emission from Water in the W3 Region
C. Wilson, A. Mason, E. Gregersen +35
We have mapped the submillimeter emission from the 1(10)-1(01) transition of ortho-water in the W3 star-forming region. A 5'x5' map of the W3 IRS4 and W3 IRS5 region reveals strong…