Lichtwechsel von λ Tauri
نویسندگان
چکیده
منابع مشابه
Modeling T Tauri Winds from He I λ 10830 Profiles
The high opacity of He I λ10830 makes it an exceptionally sensitive probe of the inner wind geometry of accreting T Tauri stars. In this line blueshifted absorption below the continuum results from simple scattering of stellar photons, a situation which is readily modeled without definite knowledge of the physical conditions and recourse to multi-level radiative transfer. We present theoretical...
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ژورنال
عنوان ژورنال: Astronomische Nachrichten
سال: 1891
ISSN: 0004-6337,1521-3994
DOI: 10.1002/asna.18911261603