Discovery of two distorted interstellar bubbles

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

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...230..782g&link_type=abstract

Astrophysical Journal, Part 1, vol. 230, June 15, 1979, p. 782-785.

Astronomy and Astrophysics

Astrophysics

25

Interstellar Gas, Nebulae, Orion Nebula, Astronomical Spectroscopy, Galactic Structure, Stellar Luminosity, Stellar Mass Ejection

Scientific paper

During an extensive program of direct imagery of emission nebulae, arcuate structures have been found around two stars. A well-defined shocklike structure is found about the T Orionis variable LL Ori, located to the side of the Orion Nebula. A less extensive shocklike structure is also found about the runaway star Zeta Oph. These structures can be best 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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