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Early stages of star formation

Different aspects of star formatlon are discussed on the basis of new submm observations. In NGC2024 slx cold (T-16K) and dense (nH“lE8-lE9cm^-3) so far unknown condensations are found and interpreted as isothermal protostars. The density and temperature structure around massive early type stars which are deeply embedded in dense regions is discussed by means of thermai
emission from dust. A star …

  • Knihovna Akademie věd České republiky (opens in new window)
  • Chini, Rolf
  • observations
  • star formation
  • interstellar material
  • model:article
  • Knihovna Akademie věd České republiky (opens in new window)
  • Chini, Rolf
  • observations
  • star formation
  • interstellar material
  • model:article
  • Česká digitální knihovna
  • http://creativecommons.org/publicdomain/mark/1.0/
  • false
  • policy:public
  • 57-62
  • Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1987 Volume:63-70 | Number:69
  • uuid:1cd551f3-41da-440c-acd3-1554bcf520b9
  • https://cdk.lib.cas.cz/client/handle/uuid:1cd551f3-41da-440c-acd3-1554bcf520b9
  • uuid:1cd551f3-41da-440c-acd3-1554bcf520b9
  • bez média
  • svazek
  • ces
  • cze
  • Czech Republic
  • 336_CZ_DigitalLibrary_article
  • 2021-06-01T12:19:28.026Z
  • 2021-06-01T12:19:28.026Z