X‐Rays from Superbubbles in the Large Magellanic Cloud. V. The HiiComplex N11
نویسندگان
چکیده
منابع مشابه
The H I Environment of Three Superbubbles in the Large Magellanic Cloud
The ambient interstellar environment of windand supernova-driven superbubbles strongly affects their evolution, but its properties are rarely well-determined. We have therefore obtained H I aperture synthesis imaging of the environment around three similar, optically-selected superbubble nebulae in the Large Magellanic Cloud. The resulting H I maps show that the ambient gas distribution around ...
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Superbubbles that result from the stellar winds and supernovae of OB associations probably play a fundamental role in the structure and energetics of the ISM in star-forming galaxies. Their influence may also dominate the relationship between the different interstellar gas phases. How do superbubbles form and evolve? How do they affect the local and global ISM? The Magellanic Clouds provide a s...
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We present Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) observations of CO J = 4 → 3 and [C I] emission in the N44 H II complex in the Large Magellanic Cloud. We detected strong CO J = 4 → 3 emission toward the H II region called as N44BC, which is located on the rim of an expanding giant shell in the N44 region. Analysis with a photodissociation region (PDR) model showed t...
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The Large Magellanic Cloud (LMC) offers an excellent laboratory to study the physical structure of the interstellar medium (ISM) because of its proximity, nearly face-on orientation, and small foreground and internal extinction. Optical and radio surveys of the LMC ISM have revealed interstellar structures of sizes ranging from a few parsecs to over 1000 parsecs. ROSAT X-ray mosaics of the LMC ...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 1998
ISSN: 0004-637X,1538-4357
DOI: 10.1086/305110