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- W2147274499 abstract "The composition and physical properties of several local clouds, including the Local Interstellar Cloud (LIC) in which the Sun is embedded, are derived from ab- sorption features in the UV spectrum of the star CMa. We derive temperatures and densities for three compo- nents by combining our interpretations of the ionization balance of magnesium and the relative population of Cii in an excited ne-structure level. We nd that for the LIC ne ~ =0 :12 0:05 cm 3 and T = 70001200 K. We derive the ionization fractions of hydrogen and discuss the ionizing processes. In particular the hydrogen and he- lium ionizations in the LIC are compatible with photoion- ization by the local EUV radiation elds from the hot stars and the cloud interface with the hot gas. We conrm the detection of high ionization species : Siiii is detected in all clouds and Civ in two of them, includ- ing the LIC, suggesting the presence of ionized interfaces around the local clouds." @default.
- W2147274499 created "2016-06-24" @default.
- W2147274499 creator A5049716126 @default.
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- W2147274499 date "2001-02-01" @default.
- W2147274499 modified "2023-09-26" @default.
- W2147274499 title "Local clouds: Ionization, temperatures, electron densities and interfaces, from GHRS and IMAPS spectra of $mathsf{epsilon}$ Canis Majoris" @default.
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- W2147274499 doi "https://doi.org/10.1051/0004-6361:20000459" @default.
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