Titlebook: Astrophysics and Space Science; Volume 255, 1997/199 John Dyson,Susan A. Lamb,P. A. Zaal Book 1998 Springer Science+Business Media New York

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The Camera Object and Flash Video,In this paper we present a comparison of the observed absorption band at about 660 cm. (15.1 μm) toward NGC7538 IRSI attributed to the bending mode of solid CO. with laboratory spectra of ion irradiated mixtures.

keloid

https://doi.org/10.1007/978-1-4302-0578-4The DEBRIS project is a search for infrared excess around Sun-like main sequence stars, and other types of stellar targets, using the Infrared Space Observatory.. Some results, calibration issues, and changes to our original program are presented. Future platforms for advancing this project after the conclusion of the ISO mission are indicated.

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1FAWN

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Relation Between Stellar Evolution and Circumstellar Processes evolution of the central body. On the contrary, during main-sequence (MS) and post-MS phases the central star determines the evolution of the circumstellar medium (CS). In these late phases the CS material can provide a most useful diagnosis on stellar evolution, particularly on the amount of mater

HILAR

Protostars and Protoplanetary Disksontinued theoretical progress, these observations have pushed our understanding of the overall star formation process to a satisfying level. We now believe that we understand the phases a dense interstellar cloud passes through in the process of becoming a young star, and we have observational examp

mastopexy

ISO Observations of Isolated Herbig AE/BE Starsrsity of emission features of carbon-rich and oxygen-rich rains. The similarity of the forsterite spectra observed for Comet Hale-Bopp and the Haebe star HD100546 is particularly striking and provides a new argument that huge comet swarms are formed in the disks surrounding young stars. While the da

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