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    • [ В начало ] Пред. | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | След.

    101. http://www.stsci.edu/institute/conference/iausps13/presentations/SpS13_program_0810.pdf
    ... Germany Aldo Serenelli, IEEC, Spain The solar CNO abundance problem CNO in photospheres of the Sun and solar-type stars CNO in massive stars Limits on solar CNO from helioseismology chair: Licai Deng Tu3 20+10 20+10 10+5 20+10 10+5 Tuesday, 16:00 - 18:00 ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/iausps13/presentations/SpS13_program_0810.pdf -- 162.9 Кб -- 05.02.2013
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    102. http://www.stsci.edu/institute/conference/iausps13/SpS13_program_0508.pdf
    ... Erlangen, Germany Aldo Serenelli, IEEC, Spain The solar CNO abundance problem CNO in photospheres of the Sun and solar-type stars CNO in massive stars Limits on solar CNO from helioseismology Session Tu3 20+10 20+10 10+5 20+10 10+5 Tuesday, 16:00 - 18:00 ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/iausps13/SpS13_program_0508.pdf -- 167.4 Кб -- 05.02.2013
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    103. http://www.stsci.edu/institute/conference/orion/orion-program.doc
    ... 10:15-10:4|Kevin Luhman |Low-Mass Stars and Brown Dwarfs in | |5 | ... 15:00-15:3|Jonathan Tan |Orion's Guide to Massive Star | |0 | |Formation | ... 0 | | | | | | | |11:00:11:3|Nino Panagia & |Low-Mass Star Formation in the | ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/orion/orion-program.doc -- 136.5 Кб -- 01.03.2014
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    104. http://www.stsci.edu/ftp/observing/status_reports/old_reports_01/hst_status_07_05_01
    ... The WF/PC-s was used to search for supernovae which have massive star progenitors ... As massive, evolved stars are the most luminous single objects in a galaxy, the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_01/hst_status_07_05_01 -- 9.4 Кб -- 05.07.2001
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    105. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_09_18_98
    ... productive direct method to determine accurate masses of stars near the end of the ... faint Companions to Pleiades Very Low-Mass Stars and Brown Dwarfs) The Near Infrared ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_09_18_98 -- 8.0 Кб -- 18.09.1998
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    106. HST this week: 140
    ... Characterizing the mass accretion rates in young low-mass stars at low metallicity . ... Are the Progenitors of SN 2002cx-like Objects Massive Stars or White Dwarfs? ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2013/thisweek140.html -- 18.7 Кб -- 13.11.2013
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    107. http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_03_11_93
    ... EST Daily Status Report as of 071/1200Z. 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed FOC/96 3591 (Massive Stars in Starburst Galaxies - FOC Images) The Faint Object Camera (f/96) was used to make observations of the star bursting galaxy IZW18 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_03_11_93 -- 4.7 Кб -- 12.03.1993
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    108. Jeff Goldader
    ... study the large-scale processes and global effects of massive star formation in galaxies, primarily using infrared observations ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/jamb98/node22.html -- 3.4 Кб -- 24.03.1998
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    109. http://www.stsci.edu/ftp/observing/status_reports/old_reports_01/hst_status_11_06_01
    ... It is proposed to determine the nature of the mass-losing star. ... Massive stars will show little {<2 mag} change in their UV luminosities during outbursts, while low-mass stars will show large ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_01/hst_status_11_06_01 -- 9.1 Кб -- 06.11.2001
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    110. HST this week: 251
    ... UV Snapshot of Low-redshift Massive Star-forming Galaxies: Searching for the Analogs of High-redshift Clumpy Galaxies . ... helium rich, and are believed to originate either from massive stars whose outer layers have been stripped through mass-loss ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2014/thisweek251.html -- 16.9 Кб -- 15.09.2014
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