... absorbing and reemitting in the infrared a considerable fraction of the stellar ... individual: WR 118 --- Stars: mass--loss --- Stars: WolfRayet --- Infrared: stars 1 ...
... The values of effective temperature of the object derived from the optical spectrum by the model atmospheres method and by modelling of spectral energy distribution in optical and infrared spectral regions agree within accuracy of methods. ...
... 1995) recently demonstrated such possibilies in a cross--identification of two large catalogs in two different frequency ranges: the IRAS (InfraRed Astronomical Satellite) Catalog (about 550.000 objects) and the UTRAO survey (about 70.000 objects) at 365 ...
... absorbing and re-emitting in the infrared a considerable fraction of the stellar ... stars: individual: WR 118 stars: massloss stars: Wolf-Rayet infrared: stars 1 ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_379_229Y.pdf -- 168.2 Кб -- 03.08.2004 Похожие документы
... Near-infrared magnitudes of the components and stellar mass estimates From published photometric data for the unresolved systems and the flux ratios measured in our speckle images, we determined the near-infrared magnitudes of the individual components. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2003/2003A&A_402_67S.pdf -- 204.3 Кб -- 01.02.2005 Похожие документы
... by IRAS (Infrared Astronomical Satellite) in 1973 and by ISO (Infrared Space ... Mid-infrared visibilities Whereas the K -band visibility traces the hot dust in the ... mid-infrared visibilities (if possible) and to fix independently the grain-size ...