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    1. Limits on the Star Formation Rates of z>2 Damped Ly Systems from H Spectroscopy
    ... Limits on the Star Formation Rates of z >2 Damped Ly Systems from H Spectroscopy . Abstract: . Introduction . ... The objective was to measure the star-formation rates in these systems. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node36.html -- 20.9 Кб -- 12.06.2006
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    2. The Formation and Evolution of LMC Rich Star Clusters: NGC 1818
    ... In brief, we will use the young clusters to constrain the star formation timescale (see below for an example) and also to look ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node27.html -- 15.4 Кб -- 12.06.2006
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    3. NICMOS Observes the Galactic Center
    ... sequence from the last episode of star formation, at searching for variability near ... Galactic Center, star formation, proper motions, variability . ... This project is meant to probe the history of star formation at the Galactic Center. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node25.html -- 12.9 Кб -- 12.06.2006
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    4. ESLAB 2007
    ... Session 1 - Stars, star formation, stellar populations and planets . 9.20 10.00 . ... Antonella Nota . Star Formation in the Small Magellanic Cloud . 12.40 13.00 . ... Tracking the distribution of Star Formation in galaxies up to z~1 . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/ESLAB2007/programme.php -- 24.7 Кб -- 01.10.2012
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    5. http://www.stecf.org/coordination/esa_eso/alma-herschel/esa-feb11-05-ver4.pdf
    ... High Redshift Galaxies and Cosmology Active Galactic Nuclei & Star Formation in Galaxies Star and Planet Formation Water in the ...
    [ 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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    6. NICMOS Science
    ... The Formation and Evolution of LMC Rich Star Clusters: NGC 1818 . ... Limits on the Star Formation Rates of z >2 Damped Ly Systems from H Spectroscopy . ... Searches for Star Formation in Damped Systems . Our Near-IR Spectroscopic Survey . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node18.html -- 15.2 Кб -- 12.06.2006
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    7. Identification and Analysis of Binary Star Systems using Probability Theory
    ... The frequency of occurrence of binary and multiple star systems remains uncertain at the present time, and is a stumbling block to our understanding of the formation of stars, stellar systems, and planetary systems. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/grochevae.html -- 17.6 Кб -- 12.06.2006
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    8. The Old Stellar Population of NGC 1569 from NICMOS data
    ... 1705 and to trace the major episodes of star formation over a Hubble time in these ... Understanding how the star formation (SF) proceeds in blue compacts and irregulars ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node29.html -- 27.6 Кб -- 12.06.2006
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    9. http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/vanderwel04.pdf
    ... formation redshift or late bursts of star formation contributing 20%­30% of the mass ... galaxies: the evolution is slow, consistent with star formation redshifts z 2 (e.g ...
    [ Текст ]  Ссылки http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/vanderwel04.pdf -- 130.5 Кб -- 16.09.2004
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    10. HST/NICMOS Observations of the Interacting System Arp 299
    ... these models we derive an age (measured from the peak of star-formation) as young as 4Myr for components C and C' in NGC 3690 ... We find that the region C+C' at the interface of the two galaxies is undergoing the youngest star-formation process. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node31.html -- 33.3 Кб -- 12.06.2006
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