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The interaction of the supernova remnant HB 21 with the interstellar medium : CO, H I, and radio continuum observations

Ken’ichi Tatematsu, Y. Fukui, T. L. Landecker, R. S. Roger

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Abstract

Les observations radio, CO et H I du reste de supernova a enveloppe evoluee, HB 21 (G 89.0+4.7), sont presentees. La morphologie de la region, les distributions des gaz moleculaires et l'interaction du reste de supernova avec la matiere interstellaire sont analysees a partir des cartes radio.

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What this paper is about

Les observations radio, CO et H I du reste de supernova a enveloppe evoluee, HB 21 (G 89.0+4.7), sont presentees. La morphologie de la region, les distributions des gaz moleculaires et l'interaction du reste de supernova avec la matiere interstellaire sont analysees a partir des cartes radio.

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OpenAlex reports 4 citations for this work. Citation counts describe recorded attention and do not establish research quality.

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Available abstract

Les observations radio, CO et H I du reste de supernova a enveloppe evoluee, HB 21 (G 89.0+4.7), sont presentees. La morphologie de la region, les distributions des gaz moleculaires et l'interaction du reste de supernova avec la matiere interstellaire sont analysees a partir des cartes radio.

Key concepts: Physics, Interstellar medium, Supernova remnant, Astrophysics, Supernova, Molecular cloud, Interstellar cloud, Astronomy

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The interaction of the supernova remnant HB 21 with the interstellar medium : CO, H I, and radio continuum observations — Research Paper | ScholarLens