Titlebook: Topics in Interstellar Matter; Invited Reviews Give Hugo Woerden (President, IAU Commission 34, 1973/7 Book 1977 D. Reidel Publishing Compa

Complement

人造

Observations of the Soft X-Ray Backgroundhat the intensity did not go to zero in the galactic plane where the absorption optical depth is very large demonstrated that they were at least partly galactic. In the last few years, several experiments have attempted to measure the X-ray shadows of the Small Magellanic Cloud, M31, and the Large M

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admission

Structure and Evolution of Wind-Driven Circumstellar Shellsre by Jenkins, the spectrometer has shown that almost all early-type stars with bolometric magnitude M. ≲ −6 have broad stellar resonance lines of N V λ1240 and O VI λ1035 that indicate stellar wind with mass loss rates Ṁ. ≳ 10. M. yr. and terminal velocities V. ≈ 1000 to 3000 km s. (Snow and Morton

恭维

Summary of Comments and Discussionon of the filling factor of the hot gas. Jenkins replied that the known irregularity in the distribution of coronal material makes a general interpretation from a single measurement untrustworthy, but the γ Cas measurement makes the notion that we are immersed in a coronal region less tenable. A com

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