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    21. http://www.stecf.org/conferences/adass/adassVII/reprints/vieirae.pdf
    ... were taken from the IUE Low-Dispersion Reference Atlas of Normal A. Stars (Heck et al. 1983), covering the wavelength range from 1150 to 3200 ° The Atlas contains 229 normal stars distributed from the spectral type O3 to K0, that were classified manually ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/vieirae.pdf -- 78.6 Кб -- 12.06.2006
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    22. NICMOS/HST H-band (F160W) Images of the 30 Dor Starburst Cluster
    ... stars have formed in the R136 cluster is key to determining whether it is a prototype young globular cluster, in which case it ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node26.html -- 13.9 Кб -- 12.06.2006
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    23. The Evolution of Stars seen with ISOCAM - the Need for NICMOS and VLT Follow...
    ... The Evolution of Stars seen with ISOCAM - the Need for NICMOS and VLT Follow Up. Abstract: . Introduction . ... 1 sees the process of stellar evolution. i) Standard staring and coronographic observations with ISOCAM towards BD+31 643 are ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node22.html -- 26.3 Кб -- 12.06.2006
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    24. http://www.stecf.org/coordination/esa_eso/alma-herschel/esa-feb11-05-ver4.pdf
    ... Star Formation in Galaxies Star and Planet Formation Water in the Universe ... Star Formation in our Galaxy We can study different stages of star formation in ... Stars In broadband continuum, ALMA should be able to detect high mass stars in our ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/esa-feb11-05-ver4.pdf -- 2622.1 Кб -- 04.09.2008
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    25. http://www.stecf.org/documents/isr/ISR_NGST_2002-02.pdf
    ... Bottom ­ the flux of the total number of galaxies and stars per unit magnitude, as a function of the K magnitude. nents (i.e., zodi, stars, galaxies) is presented in Table 1. ...
    [ Текст ]  Ссылки http://www.stecf.org/documents/isr/ISR_NGST_2002-02.pdf -- 534.3 Кб -- 11.05.2006
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    26. Future Technology
    ... Next: Design and Status of Up: No Title Previous: Limits on the Star . љ . Design and Status of the NICMOS Cryocooler . Motivations . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node37.html -- 5.7 Кб -- 12.06.2006
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    27. ALIGNASN (Nov98) --- nictools --- ALIGNASN (Nov98)
    ... The user interactively marks the stars on one direct image. ... The program first computes approximate shifts from the wcs, and then measures the coordinates of the stars using imcnt. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/nictools/alignasn.hlp.html -- 2.5 Кб -- 06.06.2006
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    28. Some Experiments with the Restoration of NICMOS Camera 2 Images of OMC-1
    ... and richly structured point-spread functions of the many bright stars in the images ... the outer frames a PSF extracted from a star in a relatively uncrowded region was ... fields with strong, varying, background lead to artifacts around bright stars ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node15.html -- 13.4 Кб -- 12.06.2006
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    29. Slitless Multiobject Spectroscopy with FOSC Type Instruments
    ... reddened OB stars, but a few are much more evolved objects, such as the WO star Sand ... star is characterized by a strong IR excess and a peculiar position in the HR ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/polcarov.html -- 14.2 Кб -- 12.06.2006
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    30. Modelling Spectro-photometric Characteristics of Eclipsing Binaries
    ... Previous: Identification and Analysis of Binary Star Systems using Probability Theory . Table of Contents -- Index -- PS reprint -- PDF reprint . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/polubekg.html -- 15.8 Кб -- 12.06.2006
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