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    1. http://www.adass.org/adass/proceedings/adass03/reprints/P10-2.pdf
    ... in the last decade, the study of very massive stars remains hampered by the lack of ... employed in the search of very massive stars, as well as in the identification of ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P10-2.pdf -- 216.0 Кб -- 27.08.2004
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    2. ADASS 2003 Conference Proceedings
    ... in the last decade, the study of very massive stars remains hampered by the lack of ... employed in the search of very massive stars, as well as in the identification of ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P10-2/ -- 13.2 Кб -- 13.08.2004
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    3. Application of the Minimum Determination Algorithm to the Study of the Fine
    ... different chemical compositions of Pop I stars were used to improve the mass-luminosity relation for stars of moderate masses ... The initial set of observational data , for the low mass stars were taken from Malkov, Piskunov, & Shpil'kina (1997). ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/malkovoy2/ -- 19.6 Кб -- 16.07.1999
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    4. Near-IR Imaging of Star-forming Regions with IRAF
    ... investigation of the gas-to-dust mass ratio, initial mass function and the star-formation efficiency in these complexes ... imaging study will allow us to search systematically for exciting sources and the low-mass stars associated with the nebul ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/chans2.html -- 7.4 Кб -- 23.06.1998
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    5. A Technique for Determining Proper Motions from Schmidt Plate Scans at ST ScI
    ... up to yr which are not listed in the Luyten or Giclas catalogues; hot DAs from the Palomar-Green (PG) Survey for J. Liebert; sdO stars in the PG survey for R. Saffer; faint, high-latitude carbon stars; and low-mass, post-AGB stars for M. Parthasarathy ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/williamsonr.html -- 10.9 Кб -- 03.11.2000
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    6. http://www.adass.org/adass/proceedings/adass03/reprints/P2-36.pdf
    ... the more massive component is a main sequence star, and the less massive secondary component is a subgiant which fills (or ... mass catalogue (Belikov 1995); Age and metallicity estimates of intermediate mass stars in eclipsing binaries (Kovaleva 2001 ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P2-36.pdf -- 96.0 Кб -- 27.08.2004
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    7. ADASS 2003 Conference Proceedings
    ... the more massive component is a main sequence star, and the less massive secondary component is a subgiant which fills (or ... mass catalogue (Belikov 1995); Age and metallicity estimates of intermediate mass stars in eclipsing binaries (Kovaleva 2001 ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P2-36/ -- 15.0 Кб -- 13.08.2004
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    8. http://www.adass.org/adass/proceedings/adass96/reprints/chans2.pdf
    ... investigation of the gas-to-dust mass ratio, initial mass function and the star-formation efficiency in these complexes ... imaging study will allow us to search systematically for exciting sources and the low-mass stars associated with the nebulФ ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/chans2.pdf -- 159.8 Кб -- 14.01.1998
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    9. Infrared Astronomy and NGST
    ... dust-enshrouded regions hiding massive star formation or active galactic nuclei ... outflow processes through which stars are built and their final masses determined ... massive envelopes of Class 0 protostars to the protoplanetary disks of pre-main ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/O2-01/ -- 37.6 Кб -- 09.10.2000
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    10. The Hubble Deep Fields
    ... than 10 point sources with and colors consistent with low-mass main sequence stars ... other HST fields) that hydrogen-burning stars with masses less than 0.3 account for ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/O1-01/ -- 37.6 Кб -- 10.10.2000
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