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K stat'e
"Some problems connected with
mass loss in late-type stars"

Primery profilei linii v spektre $\alpha$ Oriona.
Vidny effekty poglosheniya i emissii zaschet okruzhayushei obolochki (ili obolochek).
Radial'nye skorosti fotosfery byli ravny 17 km/s 12 dekabrya 1977 goda i
24 km/s v sentyabre 1974 goda.

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Astrometriya - Astronomicheskie instrumenty - Astronomicheskoe obrazovanie - Astrofizika - Istoriya astronomii - Kosmonavtika, issledovanie kosmosa - Lyubitel'skaya astronomiya - Planety i Solnechnaya sistema - Solnce

K stat'e "Some problems connected with mass loss in late-type stars"

K stat'e
"Some problems connected with
mass loss in late-type stars"