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The continuing saga of Sakurai's object (V4334 Sgr): dust production and helium line emission
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- Tyne, VH (author)
- Uppsala universitet,Institutionen för astronomi och rymdfysik
- Eyres, SPS (author)
- Geballe, TR (author)
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- Evans, A (author)
- Smalley, B (author)
- Duerbeck, HW (author)
- Asplund, M (author)
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- (creator_code:org_t)
- BLACKWELL SCIENCE LTD, 2000
- 2000
- English.
- In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. - : BLACKWELL SCIENCE LTD. - 0035-8711. ; 315:3, s. 595-599
- Journal article (peer-reviewed)
Abstract
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- We report further UKIRT spectroscopic observations of Sakurai's object (V4334 Sgr) made in 1999 April/May in the 1-4.75 mu m range, and find that the emission is dominated by amorphous carbon at T-d similar to 600 K. The estimated maximum grain size is 0.
Keyword
- stars : AGB and post-AGB; circumstellar matter; stars : individual : Sakurai's; object; stars : individual : V4334 Sgr; infrared : stars
Publication and Content Type
- ref (subject category)
- art (subject category)
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- Eyres, SPS
- Geballe, TR
- Evans, A
- Smalley, B
- Duerbeck, HW
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- Asplund, M
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