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    1. Identification and Analysis of Binary Star Systems using Probability Theory
    ... star systems remains uncertain at the present time, and is a stumbling block to our understanding of the formation of stars ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/grochevae.html -- 17.6 Кб -- 12.06.2006
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    2. Modelling Spectro-photometric Characteristics of Nonradially Pulsating Stars
    ... Modelling Spectro-photometric Characteristics of Nonradially Pulsating Stars . Abstract: . 1. Introduction . ... Next: Identification and Analysis of Binary Star Systems using Probability Theory . Up: Computational Astrophysics . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/daszynskaj.html -- 20.4 Кб -- 12.06.2006
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    3. The Formation and Evolution of LMC Rich Star Clusters: NGC 1818
    ... star formation timescale (see below for an example) and also to look for evidence of ... to detect stars on the image, and aperture photometry was obtained for these stars ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node27.html -- 15.4 Кб -- 12.06.2006
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    4. NICMOS Science
    ... A Coronagraphic Search for Substellar Companions to Young Stars . Introduction . ... Introduction . Searching around young stars . Observations with NICMOS . ... The Evolution of Stars seen with ISOCAM - the Need for NICMOS and VLT Follow Up. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node18.html -- 15.2 Кб -- 12.06.2006
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    5. Limits on the Star Formation Rates of z>2 Damped Ly Systems from H Spectroscopy
    ... The average star formation rate in each DLA depends then on their space density, so that high measured rates of star formation ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node36.html -- 20.9 Кб -- 12.06.2006
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    6. ASNPHOT (Nov98) --- nictools --- ASNPHOT (Nov98)
    ... star to be used for the photometry. ... This number corresponds to the stars marked with the asnalign task. annulus ... Calls "qphot" to perform photometry on the same star in each image of an association ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/nictools/asnphot.hlp.html -- 2.3 Кб -- 06.06.2006
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    7. NICMOS Observes the Galactic Center
    ... and/or LBV stars such as the IRS 16 stars strongly suggests that star formation has ... stars representing the tip of the main sequence from the last epoch of star ... stars with the correct properties to be the tip of the main sequence and a clump of ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node25.html -- 12.9 Кб -- 12.06.2006
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    8. ESLAB 2007
    ... 9.00 9.20 . Alvaro Gimenez . Welcome address . Session 1 - Stars, star formation, stellar populations and planets . 9.20 10.00 . Paul Crowther . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/ESLAB2007/programme.php -- 24.7 Кб -- 01.10.2012
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    9. http://www.stecf.org/conferences/adass/adassVII/reprints/grochevae.pdf
    ... star systems remains uncertain at the present time, and is a stumbling block to our ... star systems, with an estimated reliability of such identifications based on the ... stars in small area limited with angular distance for the case of a random ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/grochevae.pdf -- 112.8 Кб -- 12.06.2006
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    10. http://www.stecf.org/conferences/adass/adassVII/reprints/grochevae.ps.gz
    ... star systems remains uncertain at the present time, and is a stumbling block to our ... star systems, with an estimated reliability of such identifications based on the ... stars in small area limited with angular distance # for the case of a random ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/grochevae.ps.gz -- 100.4 Кб -- 12.06.2006
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