Titlebook: Light on Dark Matter; Proceedings of the F Frank P. Israel Conference proceedings 1986 D. Reidel Publishing Company, Dordrecht, Holland 198

Ischemia

涂掉

A Statistical Analysis of the LRS Catalogs types of spectra (LRS classes) can readily be associated with well-known groups of objects. About 96% of the sources are stars, most of them with oxygen- or carbon-rich envelopes, five sources are galaxies, and the others are compact HII regions, planetary nebulae, and ‘peculiar stars’.

Ingenuity

Spectral Decomposition of IRAS Mapsm cold interstellar dust at ~ 20 K. The confusion due to this background tends to obscure other, weaker emission, such as e.g. the emission from the shock-heated dust (T ~ 60 K) we have been looking for in supernova remnants (Braun et al 1986).

Pamphlet

Carminative

SLUMP

A Statistical Analysis and Overview of the IRAS Point Source CatalogThe IRAS Point Source Catalog can be segregated into stars, “IR galactic components”, galaxies, cirrus, and “disk and bulge stars” categories. For each source type, the types and distances of the sources are discussed, and the sky distribution, log N/log S, and identification rate are given.

谷物

The Infrared Excess From Stellar WindsThe IR excess can be used to study the density or velocity structure in the lower parts of the winds of early type stars. The depth of the emitting region and the excess in magnitudes is given for typical O-stars, as a function of λ and ?. The first results of an ongoing study of the IRAS data are discussed briefly.

陳舊

IRAS Observations of Wolf-Rayet StarsIRAS PSC, LRS, and CPC observations of Wolf-Rayet stars are used as diagnostics of hot circumstellar dust shells, cool dust in WR ring nebulae, the Ne/He abundance ratio, and the interstellar extinction. In two cases the IR energy distributions indicate WR planetary nucleus status rather than Population-I WR status.

Indebted

Astrophysics and Space Science Libraryhttp://image.papertrans.cn/l/image/586081.jpg

Kidney-Failure

978-94-010-8577-9D. Reidel Publishing Company, Dordrecht, Holland 1986