Discovery of two distorted interstellar bubbles

Details Discovery of two distorted interstellar bubbles Discovery of two distorted interstellar bubbles

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stin...7923853g&link_type=abstract

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Physics

Bubbles, Interstellar Matter, Orion Constellation, Nebulae, Spectroscopy, Stars

Scientific paper

During an extensive program of direct imagery of emission nebulae, arcuate structures were found around two stars. A well-defined shock-like structure was found about the T-Orionis variable LL Orionis, located to the side of the Orion Nebula. A less extensive shock-like structure was also found about the runaway star zeta Ophiuchus. These structures can best be described in terms of distorted interstellar bubbles. A direct consequence of this interpretation is an independent estimate of the rates of mass loss for these stars.

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