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- W4237913875 abstract "view Abstract Citations (890) References (27) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Interstellar bubbles. Castor, J. ; McCray, R. ; Weaver, R. Abstract Early-type stars blow bubbles in the interstellar medium. The radii of the bubbles are typically 30 pc. Typical conditions in their interiors are temperatures of about 1 million K and densities of about 0.01 per cu cm. The dense shell of swept-up interstellar gas that surrounds them is likely to trap the ionization front and may also have an outer layer of H2. The column density of O VI in the interior is in accord with observations by the Copernicus ultraviolet telescope. Publication: The Astrophysical Journal Pub Date: September 1975 DOI: 10.1086/181908 Bibcode: 1975ApJ...200L.107C Keywords: Bubbles; Early Stars; Interstellar Gas; Stellar Winds; Density Distribution; Gas Dynamics; Hydrogen Clouds; Interstellar Matter; Space Density; Stellar Envelopes; Stellar Evolution; Astrophysics full text sources ADS | Related Materials (1) Part 2: 1977ApJ...218..377W" @default.
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- W4237913875 date "1975-09-01" @default.
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- W4237913875 title "Interstellar bubbles" @default.
- W4237913875 doi "https://doi.org/10.1086/181908" @default.
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