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Probing Galatic ISM with halo HI clouds: the first results


Pidopryhora, Y and Liszt, H and Lockman, FJ and Rupen, M, Probing Galatic ISM with halo HI clouds: the first results, Bulletin of the American Astronomical Society, Volume 36, December 2004, pp. 1583. (2004) [Conference Extract]


Several neutral clouds in B lower Galactic halo were observed in 21 cm emission with both the GBT and the VLA D array. Because of their isolation the halo clouds give basic information on interstellar processes not available from the highly blended spectra typical of the rest of the ISM. The GBT spectra of most clouds have two line components and the VLA data show compact clumps in a more diffuse background, possibly indicating two coexisting thermal phases. As halo clouds have kinematics dominated by Galactic rotation, a reasonably accurate distance can be obtained for an individual cloud thus allowing to estimate its size and, consequently, pressure. One of the clouds lies in front of a 5.2 Jy radio continuum source (1819-096), strong enough to produce detectable absorption in the 21 cm HI line. The absorption spectrum allows to measure the cloud's opacity and spin temperature, which were found to be 0.07 and 150 K, respectively. The line also has weak wings suggesting absorption from warm HI. A ratio of observed to thermal line widths is close to unity, which indicates that the cloud may contain little turbulence.

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Item Details

Item Type:Conference Extract
Keywords:Milky Way, neutral hydrogen, HI, interstellar matter, extra-planar gas, halo clouds
Research Division:Physical Sciences
Research Group:Astronomical sciences
Research Field:Galactic astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding knowledge
Objective Field:Expanding knowledge in the physical sciences
UTAS Author:Pidopryhora, Y (Dr Yurii Pidopryhora)
ID Code:95824
Year Published:2004
Deposited By:Mathematics and Physics
Deposited On:2014-10-08
Last Modified:2014-10-09

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