Abstract
Results of IRAS observations of the Dumbbell Nebula are presented. The contribution from line emission of ions to the radiation at the four IRAS bands has been estimated. Two components of dust grains are likely to be mixed with ionized gas. The mass and temperature of dust have been estimated
Original language | English |
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Pages (from-to) | 247-251 |
Number of pages | 5 |
Journal | Astronomy & Astrophysics |
Volume | 178 |
Issue number | 1-2 |
Publication status | Published - May-1987 |