A Study on the Acceleration of the HI gas clouds around the star clusters Pleiades and H and chi Persei

Details A Study on the Acceleration of the HI gas clouds around the star clusters Pleiades and H and chi Persei A Study on the Acceleration of the HI gas clouds around the star clusters Pleiades and H and chi Persei

Dec 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968jkas....1...37y&link_type=abstract

Journal of the Korean Astronomical Society, vol. 1, no. 1, p. 37-50

Astronomy and Astrophysics

Astronomy

Scientific paper

By comparison and analysis of the optical data of the two galactic clusters of Pleiades and h and chi Persei and the radio data of the HI gas clouds which are related with those two clusters, the relative motions of those gas clouds with respect to the two clusters were obtained. The three theories on the acceleration of HI gas cloud surrounding a star cluster by Blaauw, Oort and Spitzer, and Kahn were examined with the above obtained kinetic data of the Pleiades and h and chi Persei clouds. And it was shown that Blaauw's theory is applicable to the h and chi Persei clouds but not to the Pleiades, that Oort and Spitzer's theory can explain the motions of both clouds, and that Kahn's theory needs more improvement to be a complete one.

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