Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Поиск по:www.stsci.edu/    - Поискать по всем серверам
Найдено документов: 11 ---- Время поиска: 0.30сек.   
Каталог астрономических ресурсов

  • Наблюдения, инструменты и базы данных
  • Астрометрия и служба времени
  • Небесная механика и гравиметрия
  • Теоретическая астрофизика
  • Солнечная система
  • Звезды
  • Галактики, квазары, космология
  • Исследование космоса
  • Общие вопросы
  • Прочее

  • 1 | 2 | След.

    1. http://www.stsci.edu/institute/conference/iausps13/presentations/Maehara.pdf
    ... distribution Long-term brightness variations Rotation of the star with starspots Period of brightness variation rotation period Amplitude of brightness variation size of starspots Period of brightness variation orbital period Orbital modulation of binary ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/iausps13/presentations/Maehara.pdf -- 1529.0 Кб -- 05.02.2013
    Похожие документы

    2. http://www.stsci.edu/~bond/exoticstarspaper.pdf
    ... dK star is 18% larger than a main-sequence star of the same mass, an apparent consequence of its extensive starspot coverage ...
    [ Текст ]  Ссылки http://www.stsci.edu/~bond/exoticstarspaper.pdf -- 69.3 Кб -- 17.07.2002
    Похожие документы

    3. http://www.stsci.edu/~marel/decadal/sc/153.pdf
    ... with infrared/optical spectral imaging techniques to determine the starspot distribution and 2 Figure 1: Yohkoh images of the ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/decadal/sc/153.pdf -- 197.7 Кб -- 20.02.2009
    Похожие документы

    4. IAU Symposium 258 Talks
    ... Also rotational modulated light variations indicate the presence of large starspot regions on the younger stars. ... of this program we have developed tight relations among rotation, age magnetic-activity indicators (Lx, UV emissions, starspots ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/iau258/talks -- 70.1 Кб -- 10.04.2016
    Похожие документы

    5. http://www.stsci.edu/~marel/decadal/rfi/SIMLite.pdf
    ... stable instruments can likely be built, starspots are likely to be a major ... Starspots also affect astrometry, but much less [6,7]. ... The limit of precision for RV is determined by astrophysical noise from starspots. ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/decadal/rfi/SIMLite.pdf -- 663.4 Кб -- 13.04.2009
    Похожие документы

    6. Scientific Interests of Alan D. Welty
    ... These variations are due to non-uniform photospheric temperature distributions, i.e., starspots. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~welty/welty_sci.html -- 21.5 Кб -- 11.10.2004
    Похожие документы

    7. http://www.stsci.edu/~marel/decadal/sc/352.pdf
    ... Considerable progress is being made i n mapping magnetic fields on the photospheres of magnetically active stars using rotational modulation of starspots, Doppler imaging, and Zeeman splitting (Donati et al. ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/decadal/sc/352.pdf -- 434.2 Кб -- 20.02.2009
    Похожие документы

    8. http://www.stsci.edu/hst/proposing/exp_abstract-catalogs/cy10-abstract-catalog
    ... stars are so heavily mottled by starspots that rotational modulation of their light ... the spatial distributions of the largest starspot groups have been mapped on many ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/proposing/exp_abstract-catalogs/cy10-abstract-catalog -- 289.7 Кб -- 09.04.2003
    Похожие документы

    9. http://www.stsci.edu/~golim/papers/hebb2007.pdf
    ... AU Mic exhibits quasisinusoidal variability likely due to an uneven distribution of starspots on the stellar surface. ...
    [ Текст ]  Ссылки http://www.stsci.edu/~golim/papers/hebb2007.pdf -- 1673.1 Кб -- 26.09.2007
    Похожие документы

    10. http://www.stsci.edu/ftp/ExInEd/electronic_reports_folder/TOPS.pdf
    ... If the period of stellar rotation can be determined from starspot modulation of the photometric signal or rotational modulation of the CaII H and K line emission,8 eq can be inferred from the estimated radius of that particular spectral type star, and sin ...
    [ Текст ]  Ссылки http://www.stsci.edu/ftp/ExInEd/electronic_reports_folder/TOPS.pdf -- 902.9 Кб -- 23.08.1995
    Похожие документы

    1 | 2 | След.

    Rambler's Top100 RFBR Яндекс цитирования