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Fig. 11

image

P versus θp for the stars observed towards L328. The histogram of the θp with binsize 10° are also shown. Open histogram corresponds to the θp observed on entire cloud. Filled histogram is for the θp of the stars in 10′ region around L328-IRS. Filled circles represent the values estimated for entire cloud and the filled circles enclosed within the squares show the values measures around L328-IRS. The CO outflow direction associated with L328-IRS is shown as a dashed line. The position of the Galactic plane is shown as a dotted line. A typical error-bar is shown in the figure.

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