{"title":"晚期恒星的光谱能量分布","authors":"A. M. Tatarnikov, S. G. Zheltoukhov, E. D. Malik","doi":"10.3103/S0027134924700425","DOIUrl":null,"url":null,"abstract":"<p>This paper presents a catalog of the energy distribution in the spectra of 263 stars in the wavelength range from 0.4 to 100 <span>\\(\\mu\\)</span>m, which are at late stages of evolution and have been observed by the ISO space observatory. For each object in the catalog, estimates of the observed bolometric fluxes were derived from smoothed energy distribution curves. The catalog is available at https://infra.sai.msu.ru/sai_lss_sed both as a table and in machine-readable format. It is shown that for the specified sample of objects, their ISO SWS spectra in the range 2.4–45 <span>\\(\\mu\\)</span>m correspond to the general shape of the continuum in only 60<span>\\(\\%\\)</span> of cases, and can be used without recalibration. A selection of carbon stars, accessible for the infrared observations from the MSU observatories has been made. For some of them the first brightness estimates in the <span>\\(K,L\\)</span>, and <span>\\(M\\)</span> bands were obtained with the new IR camera of the 2.5-m telescope of CMO.</p>","PeriodicalId":711,"journal":{"name":"Moscow University Physics Bulletin","volume":"79 3","pages":"385 - 392"},"PeriodicalIF":0.4000,"publicationDate":"2024-08-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Spectral Energy Distribution of Late Stage Stars\",\"authors\":\"A. M. Tatarnikov, S. G. Zheltoukhov, E. D. Malik\",\"doi\":\"10.3103/S0027134924700425\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>This paper presents a catalog of the energy distribution in the spectra of 263 stars in the wavelength range from 0.4 to 100 <span>\\\\(\\\\mu\\\\)</span>m, which are at late stages of evolution and have been observed by the ISO space observatory. For each object in the catalog, estimates of the observed bolometric fluxes were derived from smoothed energy distribution curves. The catalog is available at https://infra.sai.msu.ru/sai_lss_sed both as a table and in machine-readable format. It is shown that for the specified sample of objects, their ISO SWS spectra in the range 2.4–45 <span>\\\\(\\\\mu\\\\)</span>m correspond to the general shape of the continuum in only 60<span>\\\\(\\\\%\\\\)</span> of cases, and can be used without recalibration. A selection of carbon stars, accessible for the infrared observations from the MSU observatories has been made. For some of them the first brightness estimates in the <span>\\\\(K,L\\\\)</span>, and <span>\\\\(M\\\\)</span> bands were obtained with the new IR camera of the 2.5-m telescope of CMO.</p>\",\"PeriodicalId\":711,\"journal\":{\"name\":\"Moscow University Physics Bulletin\",\"volume\":\"79 3\",\"pages\":\"385 - 392\"},\"PeriodicalIF\":0.4000,\"publicationDate\":\"2024-08-15\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Moscow University Physics Bulletin\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.3103/S0027134924700425\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"PHYSICS, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Moscow University Physics Bulletin","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.3103/S0027134924700425","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
This paper presents a catalog of the energy distribution in the spectra of 263 stars in the wavelength range from 0.4 to 100 \(\mu\)m, which are at late stages of evolution and have been observed by the ISO space observatory. For each object in the catalog, estimates of the observed bolometric fluxes were derived from smoothed energy distribution curves. The catalog is available at https://infra.sai.msu.ru/sai_lss_sed both as a table and in machine-readable format. It is shown that for the specified sample of objects, their ISO SWS spectra in the range 2.4–45 \(\mu\)m correspond to the general shape of the continuum in only 60\(\%\) of cases, and can be used without recalibration. A selection of carbon stars, accessible for the infrared observations from the MSU observatories has been made. For some of them the first brightness estimates in the \(K,L\), and \(M\) bands were obtained with the new IR camera of the 2.5-m telescope of CMO.
期刊介绍：
Moscow University Physics Bulletin publishes original papers (reviews, articles, and brief communications) in the following fields of experimental and theoretical physics: theoretical and mathematical physics; physics of nuclei and elementary particles; radiophysics, electronics, acoustics; optics and spectroscopy; laser physics; condensed matter physics; chemical physics, physical kinetics, and plasma physics; biophysics and medical physics; astronomy, astrophysics, and cosmology; physics of the Earth’s, atmosphere, and hydrosphere.
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