Kinematics of Interstellar HI in the Region 320DEG<L<341DEG + 7DEG<B<26DEG

Details Kinematics of Interstellar HI in the Region 320DEG<L<341DEG + 7DEG<B<26DEG Kinematics of Interstellar HI in the Region 320DEG<L<341DEG + 7DEG<B<26DEG

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....94..151o&link_type=abstract

Astronomy and Astrophysics, Vol. 94, P. 151, 1981

Astronomy and Astrophysics

Astrophysics

11

Scientific paper

Hydrogen profiles are analyzed in Gaussian components in a region which includes the Lupus Loop SNR and parts of the Upper Centaurus-Lupus association and the Gould belt. It is shown that the Gould belt main H I-shell was strongly perturbed by the Lupus Loop SNR. As a consequence, three different clouds - two moving with negative velocity and a third one moving with positive velocities - seem to have separated from the main H I-shell.
Maps of the column densities and velocity distributions are given and values for the masses, momenta and energies are computed. The results imply that the Lupus Loop SNR would be located at the same distance as the association, i. e. at approximately 170 Pc from the Sun.

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