31. On the theory of ionized interstellar gas motion
نویسندگان
چکیده
منابع مشابه
Thermodynamic properties of the ionized gas 3He
In this article, we have calculated some thermodynamic properties for a system consisting of singy ionized 3He atoms and their corresponding removed electrons by employing the second quantization method at finite temperature. To perform the calculations, we have considered the kinetic term, and Coulomb interaction between the particles in our Hamiltonian. The calculated properties are free ener...
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We present Far Ultraviolet Spectroscopic Explorer (FUSE) observations of the post–asymptotic giant branch star von Zeipel 1128 (l 1⁄4 42=5, b 1⁄4 þ78=7; d 1⁄4 10:2 kpc; z 1⁄4 10:0 kpc; vLSR 1⁄4 140 8 km s 1), located in the globular cluster Messier 3. The FUSE observations cover the wavelength range 905–1187 Å at 20 km s 1 (FWHM) resolution. These data exhibit many photospheric and interstellar...
متن کاملIonized Gas in the First 10 kpc of the Interstellar Galactic Halo
We present Far Ultraviolet Spectroscopic Explorer (FUSE) observations of the post-asymptotic giant branch star von Zeipel 1128 (l = 42. 5, b = +78. 7; d = 10.2 kpc, z = 10.0 kpc; vLSR = −140± 8 km s), located in the globular cluster Messier 3. The FUSE observations cover the wavelength range 905 – 1187 Å at ∼ 20 km s (FWHM) resolution. These data exhibit many photospheric and interstellar absor...
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Aims. We present FUSE spectra of the giant H region NGC604 in the spiral galaxy M33. Chemical abundances are tentatively derived from far-UV absorption lines and compared to those derived from optical emission lines. Methods. Absorption lines from neutral hydrogen and heavy elements were observed against the continuum provided by the young massive stars embedded in the H region. the line ...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1958
ISSN: 0074-1809
DOI: 10.1017/s007418090023787x