We propose that the decline in the near-IR flux from the massive binary system g Carinae during the spectroscopic event might be explained by accreted mass that absorbs the radiation from the secondary star, and by that reduces the heating of the dust that is responsible for the near-IR emission. Th
β¦ LIBER β¦
Possible implications of mass accretion in Eta Carinae
β Scribed by Amit Kashi; Noam Soker
- Publisher
- Elsevier Science
- Year
- 2009
- Tongue
- English
- Weight
- 566 KB
- Volume
- 14
- Category
- Article
- ISSN
- 1384-1076
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