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Titlebook: Late Stages of Stellar Evolution; Proceedings of the W S. Kwok,S. R. Pottasch Conference proceedings 1987 D. Reidel Publishing Company, Dor

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發(fā)表于 2025-3-21 19:17:38 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Late Stages of Stellar Evolution
副標(biāo)題Proceedings of the W
編輯S. Kwok,S. R. Pottasch
視頻videohttp://file.papertrans.cn/582/581782/581782.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Late Stages of Stellar Evolution; Proceedings of the W S. Kwok,S. R. Pottasch Conference proceedings 1987 D. Reidel Publishing Company, Dor
描述Over the last decade we have witnessed a rapid change in our understanding of the late stages of stellar evolution. A major stimulus to this has been the synthesis of observational data from different wavebands of the electromagnetic spectrum. The advent of infrared astronomy has led to the discovery of many luminous. late-type stars obscured by their circumstellar dust envelope. Sources discovered in the IRC and AFGL infrared sky surveys were followed up by radio observa- tions, leading to the widespread use of the OH and CO molecules as probes of the circumstellar envelopes. Advances in the technique of aperture synthesis have made possible observations with unprecedent resolving power, both in spectral-line and continuum. The success of the recent IRAS sky survey, with the detection of over 250,000 sources, brings the promise of even more exciting years ahead. This area of astronomical research is also blessed with the close collaboration between theorists and observers. New ideas are constantly being quantitatively tested by new data. Theoretical predictions are eagerly used as guides for further observations. This conference was initiated with the following objective: bring to
出版日期Conference proceedings 1987
關(guān)鍵詞Bulge; CCD; Galaxy; stars; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-3813-7
isbn_softcover978-94-010-8196-2
isbn_ebook978-94-009-3813-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1987
The information of publication is updating

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1612 Mhz Survey of Selected IRAS Point Sources) . 4.0) the number of compact HII regions and galaxies sharply increases. Although the most red objects in the sample coincide with the planetair nebluae in the color-color diagram, this does not effect the statistics (none of the known nebluae were detected.).
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Conference proceedings 1987the synthesis of observational data from different wavebands of the electromagnetic spectrum. The advent of infrared astronomy has led to the discovery of many luminous. late-type stars obscured by their circumstellar dust envelope. Sources discovered in the IRC and AFGL infrared sky surveys were fo
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High Spatial Resolution Infrared Observations of Evolved Starsof their energy. They are visible at great distances in the galactic plane in spite of the effects of interstellar reddening. Many are losing mass at prodigous rates, generating thick, dusty shells of temperatures less than about 1000K. The infrared is an obvious choice for the study of photospheric and circumstellar problems alike.
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A Search for Water Maser Emission from OH/IR Stars.3-0.1, the H.O maser velocity exceeds that observed in OH. We interpret this as evidence for deviations from the expected monotonuous increase of the outflow velocity with radial distance from the star.
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Interferometric Observations of Circumstellar Envelopes at Millimeter Wavelengthsopes show a range of structures, and in one case probably demonstrate a change in the mass loss rate over time. Future studies of a wider range of objects will greatly improve our understanding of mass loss processes and the transition to the planetary nebula phase.
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